Kawai, N.,
Matsuoka, M.,
Pan, H.-C.,
Stewart, G. C..
言語
English
掲載誌/書名
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英文:
Publications of the Astronomical Society of Japan
巻, 号, ページ
Vol. 41
pp. 491-507
出版年月
1989年
出版者
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英文:
会議名称
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開催地
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アブストラクト
SS 433 was observed by Ginga for five days, and a drop in X-ray intensity centered at the phase of the optical primary minimum was detected. It is concluded that this episode was most likely an eclipse of the X-ray emitting region near the compact object by the companion star. A geometrical analysis of the binary system indicates that the X-ray source is either a fat blue-shifted jet originating from a compact object with a mass larger than 8 solar masses or, alternatively, a thin two-sided jet originating from a compact object with a mass less than 4 solar masses.
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