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一个充满活力的恒星爆发伴随着环恒星光的回声
Howard E Bond1, Arne Henden, Zoltan G Levay
1Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, Maryland 21218, USA. bond@stsci.edu
Nature
|March 28, 2003
概括
可变恒星V838 Monocerotis经历了一次独特的爆发,膨胀成一个超级巨星. 光回声显示它是银河系中最亮的恒星,表明一种新型的恒星事件.
科学领域:
- * 天文学和天体物理学
- * 恒星进化和现象
背景情况:
- *解释了恒星爆发,如新星和超新星喷射物质.
- * 介绍了V838 Monocerotis,这是一个变星,在2002年突然出现了巨大的亮度.
- * 区分V838 Mon的事件与典型的爆炸性恒星爆发.
研究的目的:
- *使用高分辨率成像和极度测量分析V838 Monocerotis的光回声.
- * 确定距离V838 Monocerotis的距离,并了解其爆发特征.
- * 调查环恒星尘埃和双星系统对恒星行为的影响.
主要方法:
- * 高分辨率的超光线光回声成像.
- * 极度测量分析光的回声.
- *光谱分析以确定二进制系统的特征.
主要成果:
- * 直接的几何距离限制设置为V838 Monocerotis (>6 kpc).
- * V838 Mon暂时成为银河系中最亮的恒星.
- * 环恒星尘埃的证据表明以前的喷发.
- *光谱数据证实V838 Mon是一个二进制星系.
结论:
- * V838 Monocerotis 代表了一种新型的恒星爆发.
- * 恒星的高亮度和不寻常的膨胀行为是无法解释的.
- * 由环恒星尘埃显示的先前喷发表明经常发生的事件.
- *二进制性质可能在独特的爆发现象中起作用.
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