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Published on: February 12, 2013
揭示了太阳附近的黑色气体的庞大云
Isabelle A Grenier1, Jean-Marc Casandjian, Régis Terrier
1Astrophysique Interactions Multi-échelles (CEA/ Universite Paris 7/CNRS), Commissanatá l'Energie Atomique, DSM/DAPNIA, Service d'Astrophysique, CEA, Saclay, 91191 Gif sur Yvette, France. isabelle.grenier@cea.fr
概括
巨大的,以前看不见的黑色气体和冷尘埃云被发现围绕着附近的分子云. 这一发现表明银河系是银河系.
科学领域:
- 天文学和天体物理学
- 星际媒介研究研究 星际媒介研究
- 天体粒子物理学的物理学
背景情况:
- 星际气体存在于原子 (HI) 和分子 (CO) 形式.
- 尘埃和玛射线提供了星际物质的替代痕迹.
- 星际介质的全部组成和结构尚未完全理解.
研究的目的:
- 调查太阳系附近"暗气体"的存在和特性.
- 了解暗气体在星际云的演化中的作用.
- 将暗气体的质量与银河系中其他气体相进行比较.
主要方法:
- 比较HI和CO线的观测结果.
- 分析尘埃的热辐射.
- 探测来自宇宙射线与气体相互作用的玛射线.
主要成果:
- 发现了广泛的冷尘和黑暗气体云.
- 这些云在HI和CO中是看不见的,但可以通过马射线检测到.
- 暗气云将密集的分子核心与更广泛的原子气体区域联系起来.
结论:
- 暗气在星际云演化中起着至关重要的作用.
- 银河系中暗气体的总质量与分子气体质量相当.
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