銀河合体
(銀河の合体 から転送)
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2022/03/28 01:07 UTC 版)
銀河合体（ぎんががったい、英語: Galaxy merger）[1]は、2つ以上の銀河が衝突する際に起こる現象である。
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- ^ a b Roukema, Boudewijn F.; Quinn, Peter J.; Peterson, Bruce A.; Rocca-Volmerange, Brigitte (December 1997). “Merging History Trees of Dark Matter Haloes: a Tool for Exploring Galaxy Formation Models”. Monthly Notices of the Royal Astronomical Society 292 (4): 835–852. arXiv:astro-ph/9707294. Bibcode: 1997MNRAS.292..835R. doi:10.1093/mnras/292.4.835.
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- ^ jgrobal
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- ^ Okamoto, Takashi; Nagashima, Masahiro (January 2001). “Morphology-Density Relation for Simulated Clusters of Galaxies in Cold Dark Matter-dominated Universes”. The Astrophysical Journal 547 (1): 109–116. arXiv:astro-ph/0004320. Bibcode: 2001ApJ...547..109O. doi:10.1086/318375.
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- ^ “Ancient Galaxy Megamergers - ALMA and APEX discover massive conglomerations of forming galaxies in early Universe”. www.eso.org. 2018年4月26日閲覧。
- ^ “Cosmic "flying V" of merging galaxies”. ESA/Hubble Picture of the Week 2013年2月12日閲覧。
[続きの解説]
- 銀河合体のページへのリンク
