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・ NGC 4102
・ NGC 4121
・ NGC 4125
・ NGC 4145
・ NGC 4151
・ NGC 4183
・ NGC 4194
・ NGC 42
・ NGC 4206
・ NGC 4214
・ NGC 4216
・ NGC 4217
・ NGC 4236
・ NGC 4244
・ NGC 4261
NGC 4262
・ NGC 428
・ NGC 4293
・ NGC 43
・ NGC 4308
・ NGC 4309
・ NGC 4314
・ NGC 4319
・ NGC 4323
・ NGC 4349-127
・ NGC 4361
・ NGC 4372
・ NGC 4395
・ NGC 44
・ NGC 4402


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NGC 4262 : ウィキペディア英語版
NGC 4262

NGC 4262 is a galaxy located in the constellation of Coma Berenices.
== Characteristics ==

NGC 4262 is a small and compact barred lenticular galaxy with a high surface brightness central bar.〔(【引用サイトリンク】publisher=NASA/IPAC Extragalactic Database (NED) )〕 It is a member of the Virgo Cluster at a distance from the Milky Way of around 50 million light-years.
It is also notable for its abundance of neutral hydrogen for a lenticular galaxy, most of it located on a ring tilted with respect to NGC 4262's galactic plane.
Studies with help of the GALEX telescope have found within that ring several clusters of young stars that can be seen on ultraviolet images.
The aforementioned ring is believed to have its origin in NGC 4262 stripping some gas of another galaxy in a close passage, likely its neighbor the spiral Messier 99

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
ウィキペディアで「NGC 4262」の詳細全文を読む



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