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在猎户座分子云表面的波浪
Olivier Berné1, Núria Marcelino, José Cernicharo
1Centro de Astrobiología, CSIC/INTA, Carretera de Torrejón a Ajalvir, km 4, 28850 Torrejón de Ardoz, Spain. berne@strw.leidenuniv.nl
Nature
|August 21, 2010
概括
天文学家在猎户座分子云的表面发现了波形结构,提供了水力动力学不稳定的第一个证据. 这些波浪很可能是凯尔文-赫尔姆霍尔茨不稳定的,是由来自大质量恒星的恒星风引起的.
科学领域:
- 天体物理学 天体物理学
- 水力动力学是指水力动力学.
- 星星形成 星星形成
背景情况:
- 大质量恒星显著影响它们周围的分子云.
- 据怀疑,水力动力学不稳定会导致云的压缩和碎片化.
- 以前对云结构的解释,如"创造的支柱",仍在争论中.
研究的目的:
- 识别和描述分子云中的水力动力学不稳定性.
- 为了找到类似波形结构的观测证据,作为这些不稳定性的标志.
主要方法:
- 观测天文学的目标是猎户座的分子云.
- 分析巨大的恒星形成区域附近的气体结构.
主要成果:
- 在猎户座分子云的表面检测到"波"的存在.
- 这些波被认为是凯尔文-赫尔姆霍尔茨不稳定的潜在特征.
- 不稳定性源于膨胀中的星云气体与先前存在的分子气体的相互作用.
结论:
- 观察到的波浪提供了分子云中水力动力学不稳定的第一个直接证据.
- 这些发现支持这样一个理论:恒星活动通过不稳定驱动云的演变.
- 这一发现为复杂的恒星形成过程提供了新的见解.
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