气候变化领域集成服务门户(CCPortal): Gas jets associated with star formation

CCPortal

DOI	10.1126/science.228.4706.1389
	Gas jets associated with star formation
	Welch W.J.; Vogel S.N.; Plambeck R.L.; Wright M.C.H.; Bieging J.H.
发表日期	1985
ISSN	0036-8075
起始页码	1389
结束页码	1395
卷号	228 期号:4706
英文摘要	Young stellar objects of both high and low luminosity emit energetic jets or winds of material that are often highly collimated and often bipolar. Near the stars, turbulent swept-up gas is observed in the emission of interstellar molecules such as carbon monoxide, and small, bright regions of water maser emission and the nebulous bright patches known as Herbig-Haro objects appear to be participating in the outflows. There are striking changes in chemical abundances associated with the attendant shocks. Probably every star goes through this phase, which may mark the end of its period of accretion.
语种	英语
来源期刊	Science
文献类型	期刊论文
条目标识符	http://gcip.llas.ac.cn/handle/2XKMVOVA/246001
作者单位	Radio Astronomy Laboratory, University of California, Berkeley, CA 94720, United States
推荐引用方式 GB/T 7714	Welch W.J.,Vogel S.N.,Plambeck R.L.,et al. Gas jets associated with star formation[J],1985,228(4706).
APA	Welch W.J.,Vogel S.N.,Plambeck R.L.,Wright M.C.H.,&Bieging J.H..(1985).Gas jets associated with star formation.Science,228(4706).
MLA	Welch W.J.,et al."Gas jets associated with star formation".Science 228.4706(1985).