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・ NGC 3486
・ NGC 35
・ NGC 2241
・ NGC 2242
・ NGC 2244
・ NGC 225
・ NGC 2257
・ NGC 2261
・ NGC 2264
・ NGC 2281
・ NGC 2291
・ NGC 2294
・ NGC 2298
・ NGC 23
・ NGC 2301
NGC 2346
・ NGC 2349
・ NGC 235
・ NGC 2354
・ NGC 2355
・ NGC 2359
・ NGC 2360
・ NGC 2362
・ NGC 2363
・ NGC 2363-V1
・ NGC 2366
・ NGC 2371-2
・ NGC 2374
・ NGC 2397
・ NGC 24


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NGC 2346 : ウィキペディア英語版
NGC 2346

NGC 2346 (also known as the Butterfly Nebula) is a planetary nebula near the celestial equator in the Monoceros constellation.〔(APOD: 28 October 2001 – NGC 2346: A Butterfly-Shaped Planetary Nebula )〕 It is bright and conspicuous and has been extensively studied. Among its most remarkable characteristics is its unusually cool central star, which is a spectroscopic binary, and its unusual shape.
The binary star, which has a period of about 16 days, is also variable, probably due to dust in orbit around it. The dust itself is heated by the central star and so NGC 2346 is unusually bright in the infrared part of the spectrum. When one of the two stars evolved into a red giant, it engulfed its companion, which stripped away a ring of material from the larger star’s atmosphere. When the red giant’s core was exposed, a fast stellar wind inflated two ‘bubbles’ from either side of the ring.
==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 2346」の詳細全文を読む



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