A0535+26 AND THE STRUCTURE OF GAS OUTFLOW FROM Be STAR
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摘要: 暂现的硬X射线双星系统中, Be星的外流气体结构是一个尚未解决的问题.本文根据Be星的观测和理论, 提出了气盘和缓慢加速星风的混合模型, 给出了速度结构, 计算了X射线光度的变化, 解释了A0535+26的许多观测现象.Abstract: In the transient hard X-ray binaries, the structure of gas outflow from Be stars is not clear. We establish a hybrid model with a disc plus gradually accelerated wind. The velocity structure is presented and the X-ray light curves are calculated. Alot of observational phenomena of A0535+26 can be explained by this model.
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