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・ NGC 4696
・ NGC 4697
・ NGC 4698
・ NGC 47
・ NGC 4700
・ NGC 4710
・ NGC 4725
・ NGC 474
・ NGC 4777
・ NGC 4780
・ NGC 4790
・ NGC 48
・ NGC 4833
・ NGC 4845
・ NGC 4866
NGC 4874
・ NGC 4881
・ NGC 4889
・ NGC 49
・ NGC 4911
・ NGC 4921
・ NGC 4945
・ NGC 4976
・ NGC 4980
・ NGC 4984
・ NGC 5
・ NGC 50
・ NGC 5001
・ NGC 5005
・ NGC 5010


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NGC 4874 : ウィキペディア英語版
NGC 4874

NGC 4874 (Coma A) is a supergiant elliptical galaxy. It was discovered by the British astronomer Frederick William Herschel I in 1785, who catalogued it as a bright patch of nebulous feature. The second brightest galaxy within the northern Coma Cluster, it is located at a distance of 109 megaparsecs (350 million light years) from Earth. Unlike a disc-shaped spiral galaxy like the Milky Way, NGC 4874 has no extensive dust lanes or spiral arms and has a smooth, featureless, ball-shaped profile that diminishes in luminosity with distance from the center. The galaxy is surrounded by an immense stellar halo that extends up to 1 million light years in diameter. It is also enveloped by a huge cloud of interstellar medium that is currently being heated by action of infalling material from its central supermassive black hole. A jet of highly energetic plasma extends out to 1,700 light years from its center.
==References==



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 4874」の詳細全文を読む



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