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在epsilon Aurigae系统中传过盘的红外图像
Brian Kloppenborg1, Robert Stencel, John D Monnier
1Department of Physics and Astronomy, University of Denver, 2112 East Wesley Avenue, Denver, Colorado 80208, USA. bkloppen@du.edu
Nature
|April 9, 2010
概括
埃普西隆·奥里盖 (Epsilon Aurigae) 罩着一个双星系统.
科学领域:
- 天文学和天体物理学
- 恒星进化 恒星进化
- 双星系统是双星系统.
背景情况:
- 埃普西隆·奥里盖 (Epsilon Aurigae) 是一个长周期的阴影二进制星系,有一个神秘的,无法检测的伴侣.
- 以前的理论表明,伴侣是一个巨大的物体,比如黑洞或红外恒星.
- 最近的假设提出了一个低质量的F型恒星,有一个遮光盘.
研究的目的:
- 为了解决围绕埃普西隆·奥里盖的伴侣的性质的190年历史的争议.
- 提供对日食物体的直接观测证据.
- 为了确定可见的F型恒星的质量.
主要方法:
- 使用干扰度成像来获得日蚀天体的直接视觉数据.
- 分析轨道元素和质量-亮度比.
- 将观察数据与现有理论模型进行比较.
主要成果:
- 直接成像证实日食物是一个不透明的,倾斜的圆盘.
- 可见的恒星是一个低质量的F型恒星 (3.6 +/- 0.7太阳质量).
- 伴星是B5V类型的,质量为5.9太阳质量.
结论:
- 发生日食的物体是一个动态上微不足道的尘埃盘,而不是一个巨大的伴侣.
- 这项研究解开了长期以来关于埃普西隆·奥里盖日食的.
- 对二进制星系的精确恒星质量已经确定.
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