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You searched for subject:(Galaxies fundamental parameters). Showing records 1 – 25 of 25 total matches.

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University of Victoria

1. Bottrell, Connor. Computational cosmology as seen through a telescope: observational properties of simulated galaxies.

Degree: Department of Physics and Astronomy, 2016, University of Victoria

 The current generation of cosmological hydrodynamical simulations offer new levels of fidelity in galaxy formation and evolution that can be benchmarked against observations. However, it… (more)

Subjects/Keywords: Galaxies; Astrophysics; Morphology; Fundamental Parameters

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APA (6th Edition):

Bottrell, C. (2016). Computational cosmology as seen through a telescope: observational properties of simulated galaxies. (Masters Thesis). University of Victoria. Retrieved from http://hdl.handle.net/1828/7467

Chicago Manual of Style (16th Edition):

Bottrell, Connor. “Computational cosmology as seen through a telescope: observational properties of simulated galaxies.” 2016. Masters Thesis, University of Victoria. Accessed November 20, 2018. http://hdl.handle.net/1828/7467.

MLA Handbook (7th Edition):

Bottrell, Connor. “Computational cosmology as seen through a telescope: observational properties of simulated galaxies.” 2016. Web. 20 Nov 2018.

Vancouver:

Bottrell C. Computational cosmology as seen through a telescope: observational properties of simulated galaxies. [Internet] [Masters thesis]. University of Victoria; 2016. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/1828/7467.

Council of Science Editors:

Bottrell C. Computational cosmology as seen through a telescope: observational properties of simulated galaxies. [Masters Thesis]. University of Victoria; 2016. Available from: http://hdl.handle.net/1828/7467


Université Paris-Sud – Paris XI

2. Salmi, Fadia. Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe.

Degree: Docteur es, Astrophysique, 2012, Université Paris-Sud – Paris XI

L'objectif de mon travail de thèse a consisté à tenter de comprendre quels sont les mécanismes principaux à l'origine de la formation d'étoiles dans les… (more)

Subjects/Keywords: Galaxies; Paramètres fondamentales – galaxies; Haut-redshift; Structure – galaxies; Évolution – galaxies : formation; Galaxies; Fundamental parameters – galaxies; High-redshift; Galaxies: structure; Galaxies: evolution – Galaxies: formation

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APA (6th Edition):

Salmi, F. (2012). Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe. (Doctoral Dissertation). Université Paris-Sud – Paris XI. Retrieved from http://www.theses.fr/2012PA112173

Chicago Manual of Style (16th Edition):

Salmi, Fadia. “Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe.” 2012. Doctoral Dissertation, Université Paris-Sud – Paris XI. Accessed November 20, 2018. http://www.theses.fr/2012PA112173.

MLA Handbook (7th Edition):

Salmi, Fadia. “Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe.” 2012. Web. 20 Nov 2018.

Vancouver:

Salmi F. Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe. [Internet] [Doctoral dissertation]. Université Paris-Sud – Paris XI; 2012. [cited 2018 Nov 20]. Available from: http://www.theses.fr/2012PA112173.

Council of Science Editors:

Salmi F. Comprendre les modes de formation d’étoiles dans l’univers lointain : Understanding the star formation modes in the distant universe. [Doctoral Dissertation]. Université Paris-Sud – Paris XI; 2012. Available from: http://www.theses.fr/2012PA112173


University of Waterloo

3. Allanson, Steven. The Star Formation Histories of Red-Sequence Galaxies.

Degree: 2009, University of Waterloo

 This thesis addresses the challenge of understanding the typical star formation histories of red sequence galaxies, using linestrength indices, mass-to-light ratios and redshift evolution as… (more)

Subjects/Keywords: galaxies: clusters; galaxies: elliptical and lenticular, cD; galaxies: stellar content; galaxies: fundamental parameters; dark matter: surveys

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APA (6th Edition):

Allanson, S. (2009). The Star Formation Histories of Red-Sequence Galaxies. (Thesis). University of Waterloo. Retrieved from http://hdl.handle.net/10012/4794

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Allanson, Steven. “The Star Formation Histories of Red-Sequence Galaxies.” 2009. Thesis, University of Waterloo. Accessed November 20, 2018. http://hdl.handle.net/10012/4794.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Allanson, Steven. “The Star Formation Histories of Red-Sequence Galaxies.” 2009. Web. 20 Nov 2018.

Vancouver:

Allanson S. The Star Formation Histories of Red-Sequence Galaxies. [Internet] [Thesis]. University of Waterloo; 2009. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10012/4794.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Allanson S. The Star Formation Histories of Red-Sequence Galaxies. [Thesis]. University of Waterloo; 2009. Available from: http://hdl.handle.net/10012/4794

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

4. Sánchez Blázquez, P. Spatially resolved star formation main sequence of galaxies in the CALIFA survey.

Degree: 2018, Institute of Physics Publishing

Subjects/Keywords: Galaxies: evolution; Galaxies: fundamental parameters; Galaxies: star formation; Física

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APA (6th Edition):

Sánchez Blázquez, P. (2018). Spatially resolved star formation main sequence of galaxies in the CALIFA survey. (Thesis). Institute of Physics Publishing. Retrieved from http://hdl.handle.net/10486/677815

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Sánchez Blázquez, P. “Spatially resolved star formation main sequence of galaxies in the CALIFA survey.” 2018. Thesis, Institute of Physics Publishing. Accessed November 20, 2018. http://hdl.handle.net/10486/677815.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Sánchez Blázquez, P. “Spatially resolved star formation main sequence of galaxies in the CALIFA survey.” 2018. Web. 20 Nov 2018.

Vancouver:

Sánchez Blázquez P. Spatially resolved star formation main sequence of galaxies in the CALIFA survey. [Internet] [Thesis]. Institute of Physics Publishing; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/677815.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Sánchez Blázquez P. Spatially resolved star formation main sequence of galaxies in the CALIFA survey. [Thesis]. Institute of Physics Publishing; 2018. Available from: http://hdl.handle.net/10486/677815

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

5. Aretxaga, Itziar. Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations.

Degree: 2018, Oxford University Press

Subjects/Keywords: Galaxies: active; Galaxies: fundamental parameters; Galaxies: photometry; Física

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APA (6th Edition):

Aretxaga, I. (2018). Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/13359

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Aretxaga, Itziar. “Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/13359.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Aretxaga, Itziar. “Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations.” 2018. Web. 20 Nov 2018.

Vancouver:

Aretxaga I. Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13359.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Aretxaga I. Broad-band and Hα surface photometry of the central regions of nearby active galaxies - I. Observations. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/13359

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of St. Andrews

6. Hill, David T. The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets .

Degree: 2011, University of St. Andrews

 Theories of how galaxies form and evolve depend greatly on constraints provided by observations. However, when those observations come from different datasets, systematic offsets may… (more)

Subjects/Keywords: Galaxies: fundamental parameters; Surveys; Techniques: photometric; Methods: observational; Methods: data analysis; Techniques: imageprocessing; Galaxies: luminosity function, mass function; Galaxies: statistics; Galaxies: structure; Infrared: galaxies

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APA (6th Edition):

Hill, D. T. (2011). The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets . (Thesis). University of St. Andrews. Retrieved from http://hdl.handle.net/10023/1696

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Hill, David T. “The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets .” 2011. Thesis, University of St. Andrews. Accessed November 20, 2018. http://hdl.handle.net/10023/1696.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Hill, David T. “The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets .” 2011. Web. 20 Nov 2018.

Vancouver:

Hill DT. The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets . [Internet] [Thesis]. University of St. Andrews; 2011. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10023/1696.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Hill DT. The optical and NIR luminous energy output of the Universe : the creation and utilisation of a 9 waveband consistent sample of galaxies using UKIDSS and SDSS observations with the GAMA and MGC spectroscopic datasets . [Thesis]. University of St. Andrews; 2011. Available from: http://hdl.handle.net/10023/1696

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of Melbourne

7. MAGOULAS, CHRISTINA. The fundamental plane and peculiar velocities from the 6dF galaxy survey.

Degree: 2012, University of Melbourne

 Early-type galaxies (ellipticals and lenticulars) are observed to populate the relation known as the Fundamental Plane that links their effective radius, Re, stellar velocity dispersion,… (more)

Subjects/Keywords: astrophysics; galaxies; early-type galaxies; elliptical and lenticular galaxies; fundamental parameters; surveys; distances and redshifts; cosmology; cosmological parameters; large-scale structure of universe

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APA (6th Edition):

MAGOULAS, C. (2012). The fundamental plane and peculiar velocities from the 6dF galaxy survey. (Doctoral Dissertation). University of Melbourne. Retrieved from http://hdl.handle.net/11343/37705

Chicago Manual of Style (16th Edition):

MAGOULAS, CHRISTINA. “The fundamental plane and peculiar velocities from the 6dF galaxy survey.” 2012. Doctoral Dissertation, University of Melbourne. Accessed November 20, 2018. http://hdl.handle.net/11343/37705.

MLA Handbook (7th Edition):

MAGOULAS, CHRISTINA. “The fundamental plane and peculiar velocities from the 6dF galaxy survey.” 2012. Web. 20 Nov 2018.

Vancouver:

MAGOULAS C. The fundamental plane and peculiar velocities from the 6dF galaxy survey. [Internet] [Doctoral dissertation]. University of Melbourne; 2012. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/11343/37705.

Council of Science Editors:

MAGOULAS C. The fundamental plane and peculiar velocities from the 6dF galaxy survey. [Doctoral Dissertation]. University of Melbourne; 2012. Available from: http://hdl.handle.net/11343/37705


University of Toronto

8. Damjanov, Ivana. Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch.

Degree: 2011, University of Toronto

The main focus of this thesis is the investigation of an interesting new population of massive passively evolving galaxies found at high redshifts. We use… (more)

Subjects/Keywords: extragalactic astronomy; galaxy evolution; elliptical galaxies; fundamental parameters; astronomical techniques; astronomical instrumentation; astrophysical data; 0606

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APA (6th Edition):

Damjanov, I. (2011). Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch. (Doctoral Dissertation). University of Toronto. Retrieved from http://hdl.handle.net/1807/31729

Chicago Manual of Style (16th Edition):

Damjanov, Ivana. “Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch.” 2011. Doctoral Dissertation, University of Toronto. Accessed November 20, 2018. http://hdl.handle.net/1807/31729.

MLA Handbook (7th Edition):

Damjanov, Ivana. “Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch.” 2011. Web. 20 Nov 2018.

Vancouver:

Damjanov I. Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch. [Internet] [Doctoral dissertation]. University of Toronto; 2011. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/1807/31729.

Council of Science Editors:

Damjanov I. Structural Evolution of Quiescent Galaxies from the Peak of the Cosmic Star Formation Epoch. [Doctoral Dissertation]. University of Toronto; 2011. Available from: http://hdl.handle.net/1807/31729


University of Nevada – Las Vegas

9. Boisvert, John Henry. How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?.

Degree: MS, Physics and Astronomy, 2013, University of Nevada – Las Vegas

  Rotation curves measured using Hi emission are a powerful tool for probing the mass distribution of galaxies. We investigate the accuracy with which rotation… (more)

Subjects/Keywords: Dark Matter; Galaxies: Fundamental Parameters; Galaxies: Individual: DDO 154; DDO 53; IC 2574; NGC 2366; NGC 3627; Galaxies: ISM; Galaxies: Kinematics & Dynamics; Astrophysics and Astronomy

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APA (6th Edition):

Boisvert, J. H. (2013). How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?. (Masters Thesis). University of Nevada – Las Vegas. Retrieved from https://digitalscholarship.unlv.edu/thesesdissertations/2820

Chicago Manual of Style (16th Edition):

Boisvert, John Henry. “How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?.” 2013. Masters Thesis, University of Nevada – Las Vegas. Accessed November 20, 2018. https://digitalscholarship.unlv.edu/thesesdissertations/2820.

MLA Handbook (7th Edition):

Boisvert, John Henry. “How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?.” 2013. Web. 20 Nov 2018.

Vancouver:

Boisvert JH. How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?. [Internet] [Masters thesis]. University of Nevada – Las Vegas; 2013. [cited 2018 Nov 20]. Available from: https://digitalscholarship.unlv.edu/thesesdissertations/2820.

Council of Science Editors:

Boisvert JH. How Accurately Can the Inclination Angle, Position Angle, and Location of the Dynamic Center be Measured from the Neutral Hydrogen Disk in the Central Regions of Dwarf Galaxies?. [Masters Thesis]. University of Nevada – Las Vegas; 2013. Available from: https://digitalscholarship.unlv.edu/thesesdissertations/2820

10. Terlevich, Roberto. The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations.

Degree: 2018, Oxford University Press

Subjects/Keywords: ISM: abundances; Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: starburst; Física

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APA (6th Edition):

Terlevich, R. (2018). The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/13375

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Terlevich, Roberto. “The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/13375.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Terlevich, Roberto. “The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations.” 2018. Web. 20 Nov 2018.

Vancouver:

Terlevich R. The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13375.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Terlevich R. The temperature and ionization structure of the emitting gas in H II galaxies: implicatins for the accuracy of abundance determinations. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/13375

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

11. Cardaci, Mónica V. Precision abundance analysis of bright H II galaxies.

Degree: 2018, Oxford University Press

Subjects/Keywords: ISM: abundances; H II regions; Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: starburst; Física

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APA (6th Edition):

Cardaci, M. V. (2018). Precision abundance analysis of bright H II galaxies. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/13391

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Cardaci, Mónica V. “Precision abundance analysis of bright H II galaxies.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/13391.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Cardaci, Mónica V. “Precision abundance analysis of bright H II galaxies.” 2018. Web. 20 Nov 2018.

Vancouver:

Cardaci MV. Precision abundance analysis of bright H II galaxies. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13391.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Cardaci MV. Precision abundance analysis of bright H II galaxies. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/13391

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

12. Sánchez-Bláquez, P. Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions.

Degree: 2018, Oxford University Press

Subjects/Keywords: Galaxies: elliptical and lenticular; Galaxies: evolution; Galaxies: fundamental parameters; Galaxies: high-redshift; Galaxies: kinematics and dynamics; Galaxies: structure; Física

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APA · Chicago · MLA · Vancouver · CSE | Export to Zotero / EndNote / Reference Manager

APA (6th Edition):

Sánchez-Bláquez, P. (2018). Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/673143

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Sánchez-Bláquez, P. “Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/673143.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Sánchez-Bláquez, P. “Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions.” 2018. Web. 20 Nov 2018.

Vancouver:

Sánchez-Bláquez P. Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/673143.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Sánchez-Bláquez P. Constraints on the evolutionary mechanisms of massive galaxies since z ~ 1 from their velocity dispersions. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/673143

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

13. Ellis, S. Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions.

Degree: 2018, EDP Sciences

Subjects/Keywords: Galaxies: ISM; Galaxies: spiral; Galaxies: evolution; Galaxies: star formation; Galaxies: fundamental parameters; Galaxies: abundances; Física

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APA (6th Edition):

Ellis, S. (2018). Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions. (Thesis). EDP Sciences. Retrieved from http://hdl.handle.net/10486/13446

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Ellis, S. “Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions.” 2018. Thesis, EDP Sciences. Accessed November 20, 2018. http://hdl.handle.net/10486/13446.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Ellis, S. “Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions.” 2018. Web. 20 Nov 2018.

Vancouver:

Ellis S. Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions. [Internet] [Thesis]. EDP Sciences; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13446.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Ellis S. Integral field spectroscopy of a sample of nearby galaxies. II. Properties of the H II regions. [Thesis]. EDP Sciences; 2018. Available from: http://hdl.handle.net/10486/13446

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

14. Sánchez Almeida, J. Do galaxies form a spectroscopic sequence?.

Degree: 2018, The American Astronomical Society; Oxford University Press

Subjects/Keywords: Galaxies: fundamental parameters; Methods: data analysis; Methods: statistical; Física

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APA (6th Edition):

Sánchez Almeida, J. (2018). Do galaxies form a spectroscopic sequence?. (Thesis). The American Astronomical Society; Oxford University Press. Retrieved from http://hdl.handle.net/10486/667040

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Sánchez Almeida, J. “Do galaxies form a spectroscopic sequence?.” 2018. Thesis, The American Astronomical Society; Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/667040.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Sánchez Almeida, J. “Do galaxies form a spectroscopic sequence?.” 2018. Web. 20 Nov 2018.

Vancouver:

Sánchez Almeida J. Do galaxies form a spectroscopic sequence?. [Internet] [Thesis]. The American Astronomical Society; Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/667040.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Sánchez Almeida J. Do galaxies form a spectroscopic sequence?. [Thesis]. The American Astronomical Society; Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/667040

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

15. Meert, Alan. Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies.

Degree: 2015, University of Pennsylvania

 We present a catalog of 2D, PSF-corrected de Vacouleurs, Sersic, de Vacouleurs + Exponential, and Sersic + Exponential fits of ~7 Ã? 105 spectroscopically selected… (more)

Subjects/Keywords: Fundamental Parameters; Galaxies; Photometry; Astrophysics and Astronomy

…237 8.8 Ser-Exp fitting parameters for disc galaxies with bar components . . . . . . 239… …galaxy parameters related to both assembly and evolution of galaxies (color, metallicity… …x29;. However, careful estimation of structural parameters for large numbers of galaxies is… …IN THE NEARBY UNIVERSE: APPLICATIONS TO EVOLUTION AND FORMATION OF GALAXIES Alan Meert… …Exponential, and S´ersic + Exponential fits of ∼ 7 × 105 spectroscopically selected galaxies drawn… 

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APA (6th Edition):

Meert, A. (2015). Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies. (Thesis). University of Pennsylvania. Retrieved from https://repository.upenn.edu/edissertations/1095

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Meert, Alan. “Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies.” 2015. Thesis, University of Pennsylvania. Accessed November 20, 2018. https://repository.upenn.edu/edissertations/1095.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Meert, Alan. “Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies.” 2015. Web. 20 Nov 2018.

Vancouver:

Meert A. Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies. [Internet] [Thesis]. University of Pennsylvania; 2015. [cited 2018 Nov 20]. Available from: https://repository.upenn.edu/edissertations/1095.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Meert A. Bulges and Disks in the Nearby Universe: Applications to Evolution and Formation of Galaxies. [Thesis]. University of Pennsylvania; 2015. Available from: https://repository.upenn.edu/edissertations/1095

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


University of Canterbury

16. Valiante, E. Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts.

Degree: Physics and Astronomy, 2014, University of Canterbury

 We present a comparison of the physical properties of a rest-frame 250μm selected sample of massive, dusty galaxies from 0 < z < 5.3. Our… (more)

Subjects/Keywords: galaxies: fundamental parameters; galaxies: evolution; galaxies: high-redshift; galaxies: ISM - ISM: dust, extinction; Submillimetre: galaxies; Field of Research::02 - Physical Sciences::0201 - Astronomical and Space Sciences::020103 - Cosmology and Extragalactic Astronomy

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APA (6th Edition):

Valiante, E. (2014). Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts. (Thesis). University of Canterbury. Retrieved from http://hdl.handle.net/10092/10492

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Valiante, E. “Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts.” 2014. Thesis, University of Canterbury. Accessed November 20, 2018. http://hdl.handle.net/10092/10492.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Valiante, E. “Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts.” 2014. Web. 20 Nov 2018.

Vancouver:

Valiante E. Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts. [Internet] [Thesis]. University of Canterbury; 2014. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10092/10492.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Valiante E. Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts. [Thesis]. University of Canterbury; 2014. Available from: http://hdl.handle.net/10092/10492

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation


Queens University

17. Hall, Christine. The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation .

Degree: Physics, Engineering Physics and Astronomy, Queens University

 The scatter of the spatially-resolved star formation main sequence (SFMS) is investigated in order to reveal signatures about processes of galaxy formation and evolution. We… (more)

Subjects/Keywords: galaxies: spiral; galaxies: star formation; galaxies: stellar content; galaxies: fundamental parameters; galaxies: photometry – surveys

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APA (6th Edition):

Hall, C. (n.d.). The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation . (Thesis). Queens University. Retrieved from http://hdl.handle.net/1974/24444

Note: this citation may be lacking information needed for this citation format:
No year of publication.
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Hall, Christine. “The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation .” Thesis, Queens University. Accessed November 20, 2018. http://hdl.handle.net/1974/24444.

Note: this citation may be lacking information needed for this citation format:
No year of publication.
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Hall, Christine. “The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation .” Web. 20 Nov 2018.

Note: this citation may be lacking information needed for this citation format:
No year of publication.

Vancouver:

Hall C. The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation . [Internet] [Thesis]. Queens University; [cited 2018 Nov 20]. Available from: http://hdl.handle.net/1974/24444.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation
No year of publication.

Council of Science Editors:

Hall C. The Scatter Dependence of the Spatially-Resolved Star Formation Main Sequence Relation . [Thesis]. Queens University; Available from: http://hdl.handle.net/1974/24444

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation
No year of publication.

18. Van de Ven, Glenn. IMF-Metallicity: A tigh local relation revealed by the CALIFA survey.

Degree: 2018, Institute of Physics Publishing

Subjects/Keywords: cD; Galaxies: elliptical and lenticular; Galaxies: evolution; Galaxies: formation; Galaxies: fundamental parameters; Galaxies: stellar content; Física

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APA (6th Edition):

Van de Ven, G. (2018). IMF-Metallicity: A tigh local relation revealed by the CALIFA survey. (Thesis). Institute of Physics Publishing. Retrieved from http://hdl.handle.net/10486/673578

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Van de Ven, Glenn. “IMF-Metallicity: A tigh local relation revealed by the CALIFA survey.” 2018. Thesis, Institute of Physics Publishing. Accessed November 20, 2018. http://hdl.handle.net/10486/673578.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Van de Ven, Glenn. “IMF-Metallicity: A tigh local relation revealed by the CALIFA survey.” 2018. Web. 20 Nov 2018.

Vancouver:

Van de Ven G. IMF-Metallicity: A tigh local relation revealed by the CALIFA survey. [Internet] [Thesis]. Institute of Physics Publishing; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/673578.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Van de Ven G. IMF-Metallicity: A tigh local relation revealed by the CALIFA survey. [Thesis]. Institute of Physics Publishing; 2018. Available from: http://hdl.handle.net/10486/673578

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

19. Bomans, D. Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?.

Degree: 2018, EDP Sciences

Subjects/Keywords: Galaxy: abundances; Galaxies: ISM; Galaxies: fundamental parameters; Galaxies: spiral; Galaxies: structure; Galaxies: evolution; Física

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APA (6th Edition):

Bomans, D. (2018). Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?. (Thesis). EDP Sciences. Retrieved from http://hdl.handle.net/10486/13448

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Bomans, D. “Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?.” 2018. Thesis, EDP Sciences. Accessed November 20, 2018. http://hdl.handle.net/10486/13448.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Bomans, D. “Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?.” 2018. Web. 20 Nov 2018.

Vancouver:

Bomans D. Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?. [Internet] [Thesis]. EDP Sciences; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13448.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Bomans D. Mass-metallicity relation explored with CALIFA. I. Is there a dependence on the star-formation rate?. [Thesis]. EDP Sciences; 2018. Available from: http://hdl.handle.net/10486/13448

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

20. Terlevich, Roberto. Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4.

Degree: 2018, Oxford University Press

Subjects/Keywords: ISM: abundances; H II regions; Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: starburst; Galaxies: stellar content; Física

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APA (6th Edition):

Terlevich, R. (2018). Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/13421

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Terlevich, Roberto. “Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/13421.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Terlevich, Roberto. “Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4.” 2018. Web. 20 Nov 2018.

Vancouver:

Terlevich R. Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13421.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Terlevich R. Abundance determination of multiple star-forming regions in the H II galaxy SDSS J165712.75+321141.4. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/13421

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

21. Morrell, Nidia. High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics.

Degree: 2018, Oxford University Press

Subjects/Keywords: ISM: abundances; H II regions; Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: individual: Haro 15; Galaxies: starburst; Física

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APA (6th Edition):

Morrell, N. (2018). High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics. (Thesis). Oxford University Press. Retrieved from http://hdl.handle.net/10486/13429

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Morrell, Nidia. “High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics.” 2018. Thesis, Oxford University Press. Accessed November 20, 2018. http://hdl.handle.net/10486/13429.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Morrell, Nidia. “High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics.” 2018. Web. 20 Nov 2018.

Vancouver:

Morrell N. High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics. [Internet] [Thesis]. Oxford University Press; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13429.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Morrell N. High-resolution spectroscopy of the blue compact dwarf galaxy Haro 15 – II. Chemodynamics. [Thesis]. Oxford University Press; 2018. Available from: http://hdl.handle.net/10486/13429

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

22. Mast, D. A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation.

Degree: 2018, American Astronomical Society

Subjects/Keywords: Galaxies: abundances; Galaxies: fundamental parameters; Galaxies: ISM; Galaxies: stellar content; Techniques: imaging spectroscopy; Física

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APA (6th Edition):

Mast, D. (2018). A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation. (Thesis). American Astronomical Society. Retrieved from http://hdl.handle.net/10486/13461

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Mast, D. “A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation.” 2018. Thesis, American Astronomical Society. Accessed November 20, 2018. http://hdl.handle.net/10486/13461.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Mast, D. “A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation.” 2018. Web. 20 Nov 2018.

Vancouver:

Mast D. A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation. [Internet] [Thesis]. American Astronomical Society; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/13461.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Mast D. A new scaling relation for the H II regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation. [Thesis]. American Astronomical Society; 2018. Available from: http://hdl.handle.net/10486/13461

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

23. Serna, Arturo. Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation.

Degree: 2018, The American Astronomical Society

Subjects/Keywords: Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: formation; Galaxies: fundamental parameters; Hydrodynamics; Methods: numerical; Física

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APA (6th Edition):

Serna, A. (2018). Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation. (Thesis). The American Astronomical Society. Retrieved from http://hdl.handle.net/10486/662080

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Serna, Arturo. “Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation.” 2018. Thesis, The American Astronomical Society. Accessed November 20, 2018. http://hdl.handle.net/10486/662080.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Serna, Arturo. “Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation.” 2018. Web. 20 Nov 2018.

Vancouver:

Serna A. Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation. [Internet] [Thesis]. The American Astronomical Society; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/662080.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Serna A. Massive galaxies at high z: Assembly patterns, structure, and dynamics in the fast phase of galaxy formation. [Thesis]. The American Astronomical Society; 2018. Available from: http://hdl.handle.net/10486/662080

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

24. Johnson, Seth Pohatan. Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies.

Degree: PhD, Astronomy, 2013, U of Massachusetts : PhD

  Comprehensive and robust analysis of galaxies found throughout cosmic time provides the means to probe the underlying characteristics of our Universe. Coupling observations and… (more)

Subjects/Keywords: galaxies - fundamental parameters; Galaxies - high redshift; Galaxies - submillimeter; methods - statistical; Astrophysics and Astronomy

fundamental parameters describing the Universe: e.g., ΩM , the density of matter (’dark matter… …59 4. X-RAY DETECTIONS OF SUB-MILLIMETER GALAXIES: ACTIVE GALACTIC NUCLEI VERSUS STARBURST… …GALAXIES . . . . . . . . 115 5.1 5.2 5.3 Introduction… …2007 parameters using least squares techniques and SATMC… …26 2.2 Comparison of input and recovered GRASIL parameters with SATMC… 

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APA (6th Edition):

Johnson, S. P. (2013). Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies. (Doctoral Dissertation). U of Massachusetts : PhD. Retrieved from https://scholarworks.umass.edu/open_access_dissertations/803

Chicago Manual of Style (16th Edition):

Johnson, Seth Pohatan. “Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies.” 2013. Doctoral Dissertation, U of Massachusetts : PhD. Accessed November 20, 2018. https://scholarworks.umass.edu/open_access_dissertations/803.

MLA Handbook (7th Edition):

Johnson, Seth Pohatan. “Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies.” 2013. Web. 20 Nov 2018.

Vancouver:

Johnson SP. Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies. [Internet] [Doctoral dissertation]. U of Massachusetts : PhD; 2013. [cited 2018 Nov 20]. Available from: https://scholarworks.umass.edu/open_access_dissertations/803.

Council of Science Editors:

Johnson SP. Characterizing Distant Galaxies: Spectral Energy Distribution Analysis of X-ray Selected Star Forming Galaxies. [Doctoral Dissertation]. U of Massachusetts : PhD; 2013. Available from: https://scholarworks.umass.edu/open_access_dissertations/803

25. Lacerda, E. A. D. The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies.

Degree: 2018, EDP Sciences

Subjects/Keywords: Galaxies: spiral; Galaxies: structure; Galaxy: evolution; Galaxy: fundamental parameters; Galaxy: stellar content; Techniques: spectroscopic; Astronomía; Física

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APA (6th Edition):

Lacerda, E. A. D. (2018). The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies. (Thesis). EDP Sciences. Retrieved from http://hdl.handle.net/10486/671065

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Chicago Manual of Style (16th Edition):

Lacerda, E A D. “The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies.” 2018. Thesis, EDP Sciences. Accessed November 20, 2018. http://hdl.handle.net/10486/671065.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

MLA Handbook (7th Edition):

Lacerda, E A D. “The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies.” 2018. Web. 20 Nov 2018.

Vancouver:

Lacerda EAD. The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies. [Internet] [Thesis]. EDP Sciences; 2018. [cited 2018 Nov 20]. Available from: http://hdl.handle.net/10486/671065.

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

Council of Science Editors:

Lacerda EAD. The CALIFA survey across the Hubble sequence: Spatially resolved stellar population properties in galaxies. [Thesis]. EDP Sciences; 2018. Available from: http://hdl.handle.net/10486/671065

Note: this citation may be lacking information needed for this citation format:
Not specified: Masters Thesis or Doctoral Dissertation

.