Volume 2 Issue 2
Apr.  1982
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Mi Guo-zhu. A MODEL OF SPORADIC STELLAR WIND INCREASE OF HARD X-RAY TRANSIENT SOURCE[J]. Chinese Journal of Space Science, 1982, 2(2): 95-103. doi: 10.11728/cjss1982.02.095
Citation: Mi Guo-zhu. A MODEL OF SPORADIC STELLAR WIND INCREASE OF HARD X-RAY TRANSIENT SOURCE[J]. Chinese Journal of Space Science, 1982, 2(2): 95-103. doi: 10.11728/cjss1982.02.095

A MODEL OF SPORADIC STELLAR WIND INCREASE OF HARD X-RAY TRANSIENT SOURCE

doi: 10.11728/cjss1982.02.095 cstr: 32142.14.cjss1982.02.095
  • Received Date: 1981-11-23
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1982-04-24
  • 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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