一个经典的新星,V2487 Oph 1998,在爆炸之前和之后的X射线中看到
Margarita Hernanz1, Glòria Sala
1Institut d'Estudis Espacials de Catalunya and Instituto de Ciencias del Espacio, Consejo Superior de Investigaciones Científicas, Gran Capità 2-4, E-08034 Barcelona, Spain. hernanz@ieec.fcr.es
概括
最近的观测表明,在 1998 年 V2487 Oph 事件发生仅 2.7 年后,经典新星爆炸的原因 - - 白矮星的积聚恢复了. 这表明新星位置之前在X射线中被观察到.
科学领域:
- * 天文学和天体物理学
- * 恒星进化和爆炸现象
背景情况:
- * 经典的新星是白矮星上热核失控的结果.
- * 了解新星爆发后的演变对于恒星物理学至关重要.
研究的目的:
- * 为了研究 1998 年的经典新星 V2487 Oph 1998 年的积累的重新建立.
- * 为了确定新星前代系统是否先前在X射线中观察到.
主要方法:
- *对1998年10月V2487的X射线多镜卫星 (XMM-Newton) 观测结果进行分析.
- *与来自Röntgen卫星 (ROSAT) 的档案数据的位置相关性.
主要成果:
- * 在爆发后2.7年,白矮星上重新建立了积累的证据.
- * 在新星的位置确定了潜在的爆发前X射线源.
结论:
- * 在经典的新星爆炸之后,积累可以相对迅速地恢复.
- *爆发前的X射线观测可能会揭示未来新星的位置.
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