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分子云磁场与M33中螺旋臂的对齐
1Max-Planck Institute for Astronomy, Königstuhl 17, D-69117 Heidelberg, Germany. li@mpia.de
Nature
|November 18, 2011
概括
银河系的磁场通过定巨大的分子云来影响恒星形成. 在银河系M33的观测显示,磁场与螺旋臂对齐,影响云结构和恒星诞生.
科学领域:
- 天体物理学 天体物理学
- 银河系的动力学
- 星星形成 星星形成
背景情况:
- 分子云形成对于恒星形成至关重要,但人们对此了解甚少.
- 大规模银河系磁场在单个云层形成中的作用受到争议.
- 动荡和旋转可能会随机化磁场,或者星系场可能会强加方向.
研究的目的:
- 为了研究银河系磁场对分子云方向的影响.
- 评估大规模磁场是否调节云积累和碎片化.
- 了解对恒星形成速度和效率的影响.
主要方法:
- 在六个巨大的分子云综合体中观察到磁场方向.
- 利用了来自附近的星系M33的数据,几乎面对面观察.
- 分析了相对于银河系结构的场面对齐.
主要成果:
- 巨大的分子云中的磁场与M33.3的螺旋臂保持一致.
- 这种对齐表明大规模银河场与云结构之间的联系.
- 这些发现支持了银河系场定分子云的假设.
结论:
- 大规模的银河磁场在组织分子云方面发挥着重要作用.
- 磁场与螺旋臂的对齐表明银河系的磁场定了这些恒星的托儿所.
- 这种定可能会影响恒星形成的速度和效率.
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