Self-consistent thermal accretion disk corona models for compact objects. II. Application to cygnus X-1

Astrophysical Journal

Volumn 487, Issue 2 PART I, 1997, Pages 759-768

  Dove, James B ^a   Wilms, Jörn ^b,c   Maisack, Michael ^b   Begelman, Mitchell C ^a  

^a UNIVERSITY OF COLORADO   (United States)

^b UNIVERSITY OF TÜBINGEN   (Germany)

^c University of Colorado   (United States)

Author keywords

Accretion, accretion disks; Radiation mechanisms: nonthermal; Radiative transfer; Stars: coronae; X rays: stars

Indexed keywords

EID: 0039874619     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/304647     Document Type: Article

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