| 硬X射线暂现源的偶发性星风增强模型 |
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| 引用本文： | 宓国柱.硬X射线暂现源的偶发性星风增强模型[J].空间科学学报,1982,2(2):95-103. |
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| 作者姓名： | 宓国柱 |
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| 作者单位： | 南京大学天文系 |
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| 摘 要： | 本文讨论了硬X射线暂现源的偶发性星风增强模型,计算了爆发期间光学光度的变化,解释了光学光度和X射线光度变化的不同步现象,结果表明这种模型可能是比较合理的。
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| 收稿时间： | 1981-11-23 |
A MODEL OF SPORADIC STELLAR WIND INCREASE OF HARD X-RAY TRANSIENT SOURCE |
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| Institution: | Department of Astronomy, Nanking University |
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| Abstract: | During the flare of hard X-ray transient source A0535 + 26 (December 1977),its optical and X-ray luminosity are non-synchronous.X-ray luminosity reached maximum about ten days later than optical luminosity did.The model of sporadic stellar wind increase of hard X-ray transient sources is discussed.The variable optical luminosity caused by the variable stellar wind is examined.The phenomenon of non-synchronism is explained in terms of this model.These come to the conclusion that the model may be reasonable |
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