Radiative–Thermal Winds from an Accretion Disk
نویسندگان
چکیده
منابع مشابه
Supernova Explosions from Accretion Disk Winds
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We present here numerical hydrodynamic simulations of line-driven accretion disk winds in cataclysmic variable systems. We calculate wind mass-loss rate, terminal velocities, and line profiles for C IV (1550 Å) for various viewing angles. The models are 2.5-dimensional, include an energy balance condition, and calculate the radiation field as a function of position near an optically thick accre...
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The effect of a possible hydrodynamical wind on the nature of hot accretion disk solutions is studied. It is found that the advection dominated branch, in the presence of a wind, maintains the self-similar solution for the disk structure with the temperature, θ ∝ 1/r, optical depth τ ∝ r and accretion rate ṁ ∝ r . Based on global solutions cooling due to wind energy loss and advection are found...
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ژورنال
عنوان ژورنال: Publications of the Astronomical Society of Japan
سال: 2002
ISSN: 0004-6264,2053-051X
DOI: 10.1093/pasj/54.3.415