CHINESE JOURNAL OF COMPUTATIONAL PHYSICS ›› 1997, Vol. 14 ›› Issue (S1): 581-583.
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Mi Guozhu1, Shen Jinying2
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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
CLC Number:
P142.6
Mi Guozhu, Shen Jinying. THE STRUCTURE OF GAS OUTFLOW DURING THE OUTBURSTS FROM VO332+53[J]. CHINESE JOURNAL OF COMPUTATIONAL PHYSICS, 1997, 14(S1): 581-583.
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http://www.cjcp.org.cn/EN/Y1997/V14/IS1/581