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维加是一个快速旋转的恒星
D M Peterson1, C A Hummel, T A Pauls
1Department of Physics and Astronomy, Stony Brook University, Stony Brook, New York 11794-3800, USA. dpeterson@astro.sunysb.edu
Nature
|April 14, 2006
概括
维加是一个快速旋转的恒星,而不是以前认为的缓慢. 新的光学干涉测量揭示了它的扭曲形状和快速旋转,解释了它不寻常的亮度和光谱线.
科学领域:
- 天文学 天文学
- 恒星天体物理学 恒星天体物理学
背景情况:
- 维加是一个主要的光谱类型标准和光度校准仪.
- 以前关于缓慢旋转的假设是基于光谱线,但异常表明旋转速度很快.
研究的目的:
- 为了调查维加的真实旋转速度和形状.
- 解决光谱数据和观测到的亮度/线形状之间的差异.
主要方法:
- 维加的光学干扰测量观测.
- 对恒星亮度分布和极轴偏移的分析.
主要成果:
- 维加正在以其破裂速度的93%旋转,看起来是扭曲的.
- 不对称的亮度和偏移的极轴证实了快速旋转.
- 解释不寻常的亮度,线形状,并预测过多的近红外辐射.
结论:
- 维加的快速旋转挑战了关于其属性的先前假设.
- 较大的表面温度差异影响了碎片盘的组成,年龄和估计值.
- 修订了对维加作为光谱和光度标准的作用的理解.
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