Comparison between two- and three-dimensional modeling of the structure of an accretion disk in a binary systemстатья
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Дата последнего поиска статьи во внешних источниках: 4 октября 2013 г.
Аннотация:We compare two- and three-dimensionalmodeling of gas-dynamical processes in the accretion
disko f a binary system. The origin of spiral waves and the loss of the angular momentum related to them are considered. It is concluded that a steady state of the diskc annot exist without taking into account the gas inflow from the donor star.