Steady models of optically thin, magnetically supported two-temperature accretion disks around a black hole

H. Oda, K. E. Nakamura, M. MacHida, R. Matsumoto

研究成果: Contribution to journalArticle

抜粋

We obtained steady solutions of optically thin two-temperature magnetized accretion disks around a black hole. We included relativistic bremsstrahlung cooling, synchrotron cooling and inverse Compton effects and assumed that the disk is threaded by toroidal magnetic field. We found that a magnetic pressure dominated new branch, which we call a low- branch, appears in the thermal equilibrium curves. The luminosity of the optically thin, magnetically supported disk can exceed 10% of the Eddington luminosity (0.1 LEdd).

元の言語英語
ページ(範囲)421-422
ページ数2
ジャーナルProceedings of the International Astronomical Union
2
発行部数S238
DOI
出版物ステータス出版済み - 8 1 2006
外部発表Yes

All Science Journal Classification (ASJC) codes

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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