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Kyoto University

1. 西野, 裕基. 宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 .

Degree: 2019, Kyoto University

Subjects/Keywords: 連星中性子星; 電波; 重力波; データ解析

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

APA (6th Edition):

西野, . (2019). 宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 . (Thesis). Kyoto University. Retrieved from http://hdl.handle.net/2433/242900

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):

西野, 裕基. “宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 .” 2019. Thesis, Kyoto University. Accessed July 20, 2019. http://hdl.handle.net/2433/242900.

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

MLA Handbook (7th Edition):

西野, 裕基. “宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 .” 2019. Web. 20 Jul 2019.

Vancouver:

西野 . 宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 . [Internet] [Thesis]. Kyoto University; 2019. [cited 2019 Jul 20]. Available from: http://hdl.handle.net/2433/242900.

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

Council of Science Editors:

西野 . 宇宙重力波干渉計LISAを用いた軌道周期が短い銀河系内の連星中性子星の観測可能性 . [Thesis]. Kyoto University; 2019. Available from: http://hdl.handle.net/2433/242900

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

.