CHINESE JOURNAL OF COMPUTATIONAL PHYSICS ›› 1997, Vol. 14 ›› Issue (S1): 581-583.

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THE STRUCTURE OF GAS OUTFLOW DURING THE OUTBURSTS FROM VO332+53

Mi Guozhu1, Shen Jinying2   

  1. 1. College of Science, Nanjing University of Aeronautics and Astronautics, 210016;
    2. School of International Business, Nanjing University, 210008
  • Received:1997-03-03 Revised:1997-05-08 Online:1997-12-25 Published:1997-12-25

Abstract: A hybrid model consisting of a gas disc plus a slowly accelerating wind is used to calculate the X-ray light curves in a Be and neutron star binary.The observational data of VO332+53 are coincident with some of them.

Key words: Be star, stellar wind, X-ray binary, X-ray burst

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