A model of sporadic stellar wind increase of hard X-ray transient source

Details A model of sporadic stellar wind increase of hard X-ray transient source A model of sporadic stellar wind increase of hard X-ray transient source

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982chjss...2...95m&link_type=abstract

Chinese Journal of Space Sciences, vol. 2, April 1982, p. 95-103. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

Astronomical Models, Stellar Flares, Stellar Winds, X Ray Sources, Radiant Heating, Stellar Luminosity, Stellar Models, Transient Response

Scientific paper

During the flare of hard X-ray transient source A0535+26 (December 1977), its optical and X-ray luminosity are nonsynchronous. 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 nonsynchronism is explained in terms of this model. It is concluded that the model may be reasonable.

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