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Circinus Galaxy
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Circinus Galaxy : ウィキペディア英語版
Circinus Galaxy

The Circinus Galaxy (ESO 97-G13) is a Seyfert galaxy〔(【引用サイトリンク】 work=Results for ESO 97-13 )〕 in the Circinus constellation - and one of the closest to our Milky Way(see also NGC 185). It is only 4 degrees below the Galactic plane, and 13 million light-years away. The galaxy is undergoing tumultuous changes, as rings of gas are being ejected from the galaxy. The outermost ring is 700 light-years from the center of the galaxy and the inner ring is 130 light-years out. The Circinus galaxy can be seen using a small telescope, however it was not noticed until 25 years ago because it was obscured by material from our own galaxy. The Circinus Galaxy is a Type II Seyfert galaxy and is one of the closest known active galaxies to the Milky Way, though it is probably slightly further away than Centaurus A.
Circinus Galaxy was a home for SN 1996cr, that has been identified over a decade after it exploded. The supernova was first singled out in 2001 as a bright,
variable object in a
Chandra image,
but it was not confirmed as a supernova until years later.
==References==


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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