密集分子云的质量密度特征的演变
S Donkov1, I Zh Stefanov2, T V Veltchev3
1Institute of Astronomy and NAO, Bulgarian Academy of Sciences, 72 Tzarigradsko Chausee Boulevard, 1784 Sofia, Bulgaria.
Physical review. E
|June 19, 2025
概括
研究人员得出了分子云密度演变的方程,找到一个稳定的,可观测的密度配置指数2远离中心.
科学领域:
- 天体物理学 天体物理学
- 计算流体动力学的流体动力学.
背景情况:
- 密集的分子云对于恒星形成至关重要.
- 了解它们的内部动态,特别是质量积累,是关键.
研究的目的:
- 在密集的分子云中导出质量密度特征演变的指导方程.
- 根据积累流来分析云层的稳定性.
主要方法:
- 应用水力动力学到一个自我引力,同热,球形气体云模型.
- 导出了一个非线性偏微分方程系统,用于密度配置指数和增积速度.
- 利用稳定状态流量假设和领先顺序术语分析来获得近似的解决方案.
主要成果:
- 获得密度特征 (距离中心远的ρ=l−2,距离中心近的ρ=l−3/2) 和增积速度的近似解.
- 确认与之前工作中的节能方程一致.
- 确定外层仅在次声波积累流中是稳定的.
结论:
- 远离中心观察到的2的密度缩放指数是一种吸引力,应该在密集的分子云中可以观察到.
- 亚声波积累流对于外层云层的动态稳定性是必要的.
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