Stellar-Mass Black-Hole Models at Eddington Luminosity(Poster)
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概要
- 論文の詳細を見る
Black-hole accretion disk models with 3 and 15 Eddington critical accretion rates are examined by two-dimensional radiation hydrodynamic calculations. The numerical results show that the super-Eddington model with 15 Eddington critical rate can explain well the small collimation degree of the jets and the high mass-outflow rate estimated for SS 433.
- 理論物理学刊行会の論文
- 2004-11-15
著者
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Okuda T
Otemae College Of Nutrition
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Ohnuki T
Sankyo Co. Ltd. Tokyo Jpn
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Otake Toru
Otemae College Of Nutrition
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Okuda Toru
Hakodate College Hokkaido University Of Education
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