A Transition Disk Model for Cygnus X-1-Reference-Cited by-同舟云学术

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A Transition Disk Model for Cygnus X-1

Published:1996-08 Issue: Volume:467 Page:405
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Misra Ranjeev,Melia Fulvio

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 16 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Thermal Conduction and Hydrodynamical Winds in Magnetized Viscous Accretion Disk Dynamics;2024

2. The broad-band spectrum of Cygnus X-1 measured by INTEGRAL;Astronomy & Astrophysics;2006-01-13

3. The Effect of a Dissipative Corona on the Structure and Stability of Cold Optically Thick Accretion Disks at High Accretion Rates;The Astrophysical Journal;2002-07-10

4. The Influence of Hydrodynamical Winds on Hot Accretion Disk Solutions;The Astrophysical Journal;2001-06

5. A High‐Sensitivity Measurement of the MeV Gamma‐Ray Spectrum of Cygnus X‐1;The Astrophysical Journal;2000-11-10

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