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L1448-IRS2E : ウィキペディア英語版
L1448-IRS2E
L1488-IRS2E is an object located in the Perseus star forming region. A clump of dense gas and dust, L1488-IRS2E is one-tenth as luminous as our sun and thus is unlikely to be a true protostar at this time. However, its density is high enough that it is ejecting streams of matter from itself, and so it is a likely candidate for the first discovered core in hydrostatic quasi-equilibrium. This would mean that L1488-IRS2E represents an early phase in stellar development which has so far remained unobserved due to the short time that a star spends in this phase and the low luminosity which comes from a star not yet developed past it.
==External links==

* http://arxiv.org/abs/1004.2443
* http://www.spacedaily.com/reports/Astronomers_Witness_A_Star_Being_Born_999.html
* http://www.brightsurf.com/news/headlines/56409/Astronomers_Witness_a_Star_Being_Born.html


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「L1448-IRS2E」の詳細全文を読む



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