A 0535 + 26 and the structure of gas outflow from Be stars

Details A 0535 + 26 and the structure of gas outflow from Be stars A 0535 + 26 and the structure of gas outflow from Be stars

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989chjss...9r.161m&link_type=abstract

Chinese Journal of Space Science (ISSN 0254-6124), vol. 9, July 1989, p. 161-167. In Chinese, with abstract in English.

Physics

B Stars, Stellar Winds, X Ray Binaries, Light Curve, Stellar Models

Scientific paper

In the transient hard X-ray binaries, the structure of gas outflow from
Be stars is not clear. A hybrid model with a disk and a gradually
accelerated wind is established. The velocity structure is presented and
the X-ray light curves are calculated. A number of observational
phenomena of A 0535 + 26 can be explained by this model.

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