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大颗粒细胞在巨星 π1 的表面
C Paladini1,2, F Baron3, A Jorissen1
1Institut d'Astronomie et d'Astrophysique, Université libre de Bruxelles, CP 226, 1050 Bruxelles, Belgium.
Nature
|December 21, 2017
概括
研究人员对已发展的巨星 π1 Gruis 的表面进行了成像,揭示了大型的对流细胞. 这些发现与恒星对流的模拟相一致,为天体物理过程提供了新的见解.
科学领域:
- 天体物理学
- 恒星演变
- 血物理
背景情况:
- 在恒星,尘埃云和棕矮星中,对流动至关重要.
- 太阳颗粒提供了恒星对流的模型,但巨星由于重力较低而表现出不同的尺度.
- 由于尘埃掩盖了它们的表面,因此很难研究进化巨星的对流.
研究的目的:
- 在进化的巨星上描述对流.
- 为了研究对流细胞的物理起源.
- 将观测与恒星对流模拟进行比较.
主要方法:
- 进化巨星 π1 Gruis 的干扰度成像.
- 分析恒星的无尘大气和分子不透明度.
- 测量强度对比度和颗粒大小.
主要成果:
- 直接成像揭示了 π1 Gruis 的复杂的对流模式.
- 观察到平均强度对比度为12%,在较短的波长时增加.
- 它的特征颗粒大小为1.2 × 1011米 (占恒星直径的27%).
结论:
- 观察到的 π1 Gruis 的对流性质与理论缩放关系一致.
- 这项研究提供了大规模对流的直接证据.
- 这些发现增强了我们对太阳之外的天体物理对流的理解.
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