Physics of Flares in Black Hole Microquasar V4641 Sgr(Poster)
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概要
- 論文の詳細を見る
We present a time-dependent disk instability model for short duration flare events observed in the black hole microquasar V4641 Sgr = SAX J1819.3-2525. To reproduce the observed short duration of the flare, a ring-like, truncated Keplerian disk is required to reproduce the observed flares of a few day duration.
- 2004-11-15
著者
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Mineshige S
Kyoto Univ. Kyoto
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Mineshige Shin
Yukawa Institute For Theoretical Physics Kyoto University
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MATSUSHITA Satoki
Academia Sinica, Institute of Astronomy and Astrophysics
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Sameshima Masahiro
Institute Of Astronomy The University Of Tokyo
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Kim Soon-wook
Department Of Astronomy And Space Science Chungnam National University
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Sumiyoshi Masanao
Kyoto Univ. Kyoto
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Mineshige Shin
Kyoto Univ. Kyoto
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MINESHIGE Shin
Department of Astronomy, Graduate School of Science Kyoto University
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