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Be/X射线双星的多波段研究

Be/X射线双星的多波段研究

Be/X射线双星的多波段研究

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结论: 在A0535+26中,每次较强的X射线爆发都发生在系统光学光度下降<br />

的过程当中,2009年我们观测到的Halpha强度和V星等之间的逆相关变化<br />

同样也说明星周盘的内区一个低密度区域的形成,它和<strong>Be</strong>星的物质喷发活动<br />

有关。

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