Radioactive Al-26 from the Scorpius-Centaurus association

	Radioactive Al-26 from the Scorpius-Centaurus association
	Diehl, R.1; Lang, M. G.1; Martin, P.1; Ohlendorf, H.1; Preibisch, Th.2; Voss, R.1,4; Jean, P.5; Roques, J. -P.5; von Ballmoos, P.5; Wang, W.3
刊名	ASTRONOMY & ASTROPHYSICS
	2010-11-01
卷号	522
关键词	stars: massive supernovae: general evolution solar neighborhood gamma rays: ISM
英文摘要	Context. The Scorpius-Centaurus association is the most-nearby group of massive and young stars. As nuclear-fusion products are ejected by massive stars and supernovae into the surrounding interstellar medium, the search for characteristic gamma-ray from radioactivity is one way to probe the history of activity of such nearby massive stars on a My time scale through their nucleosynthesis. Al-26 decays with a radioactivity lifetime tau similar to 1 My, 1809 keV gamma-rays from its decay can be measured with current gamma-ray telescopes.
收录类别	SCI
语种	英语
WOS记录号	WOS:000284153100057
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/7749]
专题	国家天文台_光学天文研究部
作者单位	1.Max Planck Inst Extraterr Phys, D-85741 Garching, Germany 2.Univ Sternwarte, D-81679 Munich, Germany 3.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China 4.Excellence Cluster Origin & Struct Universe, D-85748 Garching, Germany 5.Ctr Etud Spatiale Rayonnements, F-31028 Toulouse 4, France
推荐引用方式 GB/T 7714	Diehl, R.,Lang, M. G.,Martin, P.,et al. Radioactive Al-26 from the Scorpius-Centaurus association[J]. ASTRONOMY & ASTROPHYSICS,2010,522.
APA	Diehl, R..,Lang, M. G..,Martin, P..,Ohlendorf, H..,Preibisch, Th..,...&Wang, W..(2010).Radioactive Al-26 from the Scorpius-Centaurus association.ASTRONOMY & ASTROPHYSICS,522.
MLA	Diehl, R.,et al."Radioactive Al-26 from the Scorpius-Centaurus association".ASTRONOMY & ASTROPHYSICS 522(2010).