Volume 9 Issue 3
Aug.  1989
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Mi Guo-zhu, Shen Jin-ying. A0535+26 AND THE STRUCTURE OF GAS OUTFLOW FROM Be STAR[J]. Chinese Journal of Space Science, 1989, 9(3): 161-167. doi: 10.11728/cjss1989.03.161
Citation: Mi Guo-zhu, Shen Jin-ying. A0535+26 AND THE STRUCTURE OF GAS OUTFLOW FROM Be STAR[J]. Chinese Journal of Space Science, 1989, 9(3): 161-167. doi: 10.11728/cjss1989.03.161

A0535+26 AND THE STRUCTURE OF GAS OUTFLOW FROM Be STAR

doi: 10.11728/cjss1989.03.161
  • Received Date: 1989-01-19
  • Rev Recd Date: 1900-01-01
  • Publish Date: 1989-08-24
  • 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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