{{ Galaxy |
| name =大犬座矮星系
| epoch = J2000
| type = 不規則
| ra =
| dec = 。一些研究表明，恆星的蹤跡實際上是扭曲的星系薄盤和厚盤族群的一部分，而不是銀河系與矮橢球星系碰撞的結果。2009年對該地區的調查只發現了十顆天琴座RR型變星，這與銀河系的銀暈和厚盤的族群一致，而不像是一個單獨的矮橢球星系。
相關條目
- 梅西爾 79
- 半人馬座ω星團
- 星系的形成和演化
參考資料
- N. F. Martin, R. A. Ibata, M. Bellazzini, M. J. Irwin, G. F. Lewis, W. Dehnen, (February 2004). [http://xxx.lanl.gov/abs/astro-ph/0311010 A dwarf galaxy remnant in Canis Major: the fossil of an in-plane accretion onto the Milky Way.] Monthly Notices of the Royal Astronomical Society 348 (1) 12.
- [https://web.archive.org/web/20080527020725/http://astro.u-strasbg.fr/images_ri/canm-e.html Official press release announcing discovery (University of Strasbourg)]
- [https://web.archive.org/web/20070714155533/http://www.seds.org/messier/more/cma_dw.html SEDS page on the Canis Major dwarf galaxy]
外部連結
- [https://web.archive.org/web/20090114035201/http://www.skynightly.com/reports/Deriving_The_Shape_Of_The_Galactic_Stellar_Disc.html Deriving The Shape Of The Galactic Stellar Disc] (SkyNightly) Mar 17, 2006
- [http://messier.seds.org/more/cma_dw.html SEDS page on the Canis Major dwarf galaxy]
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