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
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
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.