The direct problem for two-dimensional transonic outflow of gas from the surface of a slowly-rotating star

Details The direct problem for two-dimensional transonic outflow of gas from the surface of a slowly-rotating star The direct problem for two-dimensional transonic outflow of gas from the surface of a slowly-rotating star

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998arep...42...71b&link_type=abstract

Astronomy Reports, Volume 42, Issue 1, January 1998, pp.71-80

Astronomy and Astrophysics

Astronomy

Scientific paper

A procedure for solving the direct problem for the case of transonic outflow of gas from the surface of a slowly rotating star is formulated in the framework of ideal, two-dimensional hydrodynamics. This is possible because of the existence of a previously known exact analytical solution - that for spherically-symmetric stellar wind. Analytical expressions for the stream function, gas density, velocity, etc. are obtained for asymptotically distant regions. The solution displays a tendency for the formation of a disk in the equatorial plane.

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