TY  - CHAP
A1  - Votruba, V.
A1  - Feldmeier, Achim
A1  - Kubát, Jiří
A1  - Rätzel, D.
T1  - Multicomponent stellar wind of hot stars
N2  - We developed a time-dependent multicomponent hydrodynamical code for simulation of the stellar wind from hot stars and applied it to stars with high and low density winds.
Y1  - 2007
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus-17677
ER  - 
TY  - CHAP
A1  - Kusterer, D.-J.
A1  - Nagel, T.
A1  - Werner, K.
A1  - Feldmeier, Achim
T1  - Radiative transfer in CV disk winds
N2  - Mass accretion onto compact objects through accretion disks is a common phenomenon in the universe. It is seen in all energy domains from active galactic nuclei through cataclysmic variables (CVs) to young stellar objects. Because CVs are fairly easy to observe, they provide an ideal opportunity to study accretion disks in great detail and thus help us to understand accretion also in other energy ranges. Mass accretion in these objects is often accompanied by mass outflow from the disks. This accretion disk wind, at least in CVs, is thought to be radiatively driven, similar to O star winds. WOMPAT, a 3-D Monte Carlo radiative transfer code for accretion disk winds of CVs is presented.
Y1  - 2007
U6  - http://nbn-resolving.de/urn/resolver.pl?urn:nbn:de:kobv:517-opus-17847
ER  -