Spectroscopy of the Stellar Wind in the Cygnus X-1 System

The X-ray luminosity of black holes is produced through the accretion of material from their companion stars. Depending on the mass of the donor star, accretion of the material falling onto the black hole through the inner Lagrange point of the system or accretion by the strong stellar wind can occu...

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Bibliographic Details
Main Authors: I. Miškovičová, M. Hanke, J. Wilms, M. A. Nowak, K. Pottschmidt, N. S. Schulz
Format: Article
Language:English
Published: CTU Central Library 2011-01-01
Series:Acta Polytechnica
Subjects:
Online Access:https://ojs.cvut.cz/ojs/index.php/ap/article/view/1332