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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
来自一个年轻的大质量星系的全银河系超级风的发现,红移z大约为3,来自一个全银河系超级风
R J Wilman1, J Gerssen, R G Bower
1Department of Physics, University of Durham, South Road, Durham DH1 3LE, UK. r.j.wilman@durham.ac.uk
Nature
|July 15, 2005
概括
高速度的星系外流会影响整个星系,而不仅仅是恒星形成区域. 观测显示,一个星系喷射出广泛,连贯的气体屏幕,证明了超级风在整个星系的影响.
科学领域:
- 宇宙进化的宇宙进化.
- 银河系的形成和演变.
- 天体物理学 天体物理学
背景情况:
- 银河系外流对于银河系进化理论至关重要,它调节恒星形成并丰富银河间介质.
- 之前对高红移星系的观测不清楚这些外流的空间范围.
研究的目的:
- 为了研究高红移银河系中高速银河系外流的空间范围和影响.
- 为了确定外流是否影响整个银河系或是局部.
主要方法:
- 一个恒星形成星系的二维光谱在红移z=3.09时.
- 对空间扩展的Lyalpha线辐射和H i吸收的分析.
- 测量吸收气体屏幕的横向延伸和速度连贯性.
主要成果:
- 观测到一个星系在z=3.09的空间扩展的Lyalpha辐射.
- 发现该辐射被前景HI屏幕所吸收,覆盖了整个银河系.
- 屏幕的横向延伸至少为100 kpc,并且显示出了显著的速度连贯性.
- 这块屏幕在过去的星球爆发中从银河系中弹出,并席卷了星系间介质.
结论:
- 高速度的银河系外流,或超级风,对整个银河系产生影响.
- 这些外流可以显著影响银河系及其周围的星系间介质.
- 观察到的现象证明了早期宇宙中星爆驱动的外流的大规模后果.
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