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UGC 4879
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UGC 4879 : ウィキペディア英語版
UGC 4879

UGC 4879, which is also known as VV 124, is the most isolated dwarf galaxy in the periphery of the Local Group. It is an irregular galaxy at a distance of 1.38 Mpc. Low-resolution spectroscopy yielded inconsistent radial velocities for different components of the galaxy, hinting at the presence of a circumstellar disk. There is also evidence of this galaxy containing dark matter.
==Appearance==
UGC 4879 is a transition type galaxy, meaning it has no rings (Denoted rs). It is also a spheroidal (dSph) galaxy, meaning it has a low luminosity. It has little to no gas or dust, or recent star formation. It is also irregular, meaning it has no specific form.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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