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银河中心附近的磁扭曲波被"双螺旋"星云所追踪
Mark Morris1, Keven Uchida, Tuan Do
1Department of Physics and Astronomy, University of California, Los Angeles, California 90095-1547, USA. morris@astro.ucla.edu
Nature
|March 17, 2006
概括
天文学家在银河系中心附近发现了一个独特的双螺旋红外星云. 这种结构被解释为强大的磁波,可能会影响银河系现象.
科学领域:
- * 天体物理学 * 天体物理学
- * 银河系动力学 银河系动力学
- * 等离子体物理学
背景情况:
- *银河系的中心磁场很强 (高达1毫瓦斯),并且具有双极几何.
- * 了解这个场对于它对分子云,恒星形成和银河系风的影响至关重要.
- *以前的研究已经描述了一般的磁场,但缺乏详细的结构.
研究的目的:
- * 为了研究和描述银河中心磁场内的不寻常结构.
- * 解释最近观察到的双螺旋星云的形成和性质.
- * 了解星云与中央磁性气体盘之间的关系.
主要方法:
- * 红外观测被用来探测和成像星云.
- * 对观察到的结构进行了形态分析.
- * 应用了基于磁动力学的理论解释.
主要成果:
- *发现一个具有交织的双螺旋形态的红外星云.
- * 星云位于距离银河系中心大约100帕塞克,其轴垂直于银河系平面.
- * 观测到的结构跨越25个帕塞克,表现出两个螺旋链的1.25个全转.
结论:
- * 双螺旋星云被解释为扭曲的阿尔夫恩波.
- * 这波可能是由磁化环核气体盘的旋转驱动的.
- *观察到环核盘与螺旋之间的可能连接通道,需要进一步研究.
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