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2001MNRAS.324..319L - Mon. Not. R. Astron. Soc., 324, 319-324 (2001/June-3)
Hydrodynamical winds from two-temperature plasma in X-ray binaries.
LIN D.J., MISRA R. and TAAM R.E.
Abstract (from CDS):
The results are applied to black hole candidate X-ray binary systems in the hard spectral state (Cyg X-1, GX 339-4 and Nova Muscae), and it is found that the inferred optical depth (τ) is similar to τc, suggesting that they are wind-regulated systems. On the other hand, for X-ray binary systems containing a neutron star (e.g., Cyg X-2) τ is much larger than τc indicating the absence of significant hydrodynamical winds.
Abstract Copyright: The Royal Astronomical Society
Journal keyword(s): accretion, accretion discs - black hole physics - hydrodynamics
Simbad objects: 12
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