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Words near each other
・ NGC 7499
・ NGC 75
・ NGC 7510
・ NGC 752
・ NGC 7522
・ NGC 7537
・ NGC 7538
・ NGC 76
・ NGC 7600
・ NGC 7635
・ NGC 7662
・ NGC 7673
・ NGC 7686
・ NGC 77
・ NGC 7714
NGC 772
・ NGC 7727
・ NGC 7742
・ NGC 7752 and NGC 7753
・ NGC 7759
・ NGC 7777
・ NGC 7789
・ NGC 7790
・ NGC 7793
・ NGC 78
・ NGC 7814
・ NGC 7822
・ NGC 784
・ NGC 7840
・ NGC 79


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NGC 772 : ウィキペディア英語版
NGC 772

NGC 772 (also known as ''Arp 78'') is an unbarred spiral galaxy approximately 130 million light-years away in the constellation Aries.
== Characteristics ==

Around 200,000 light years in diameter, NGC 772 is twice the size of the Milky Way Galaxy, and is surrounded by several satellite galaxies – including the dwarf elliptical, NGC 770 – whose tidal forces on the larger galaxy have likely caused the emergence of a single elongated outer spiral arm that is much more developed than the others arms. Halton Arp includes NGC 772 in his Atlas of Peculiar Galaxies as Arp 78, where it is described as a "Spiral galaxy with a small high-surface brightness companion".
Two supernovae (SN 2003 hl & SN 2003 iq) have been observed in NGC 772.
NGC 772 probably has a H II nucleus, but it may be a transitional object.

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 772」の詳細全文を読む



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