Accretion Disk Boundary Layers: Their Structure and Stability
نویسندگان
چکیده
منابع مشابه
Accretion disk boundary layers in classical TTauri stars
The dynamical and thermal structure of an opaque boundary layer, connecting a classical T Tauri star (CTTS: M∗ = 1M , R∗ = 4.3R , Teff = 5000K) with its accretion disk (Ṁ = 10−7M /yr), has been computed, including particularly the effect of a turbulence-driven global heat transport. The inner boundary has been shifted deeper and deeper into the star’s envelope in order to determine how this aff...
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ژورنال
عنوان ژورنال: International Astronomical Union Colloquium
سال: 1987
ISSN: 0252-9211
DOI: 10.1017/s0252921100105020