Radiative Transfer in circumstellar envelopes of Variable Mass Loss Rate

Details Radiative Transfer in circumstellar envelopes of Variable Mass Loss Rate Radiative Transfer in circumstellar envelopes of Variable Mass Loss Rate

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aas...197.0810n&link_type=abstract

American Astronomical Society, 197th AAS Meeting, #08.10; Bulletin of the American Astronomical Society, Vol. 32, p.1407

Astronomy and Astrophysics

Astronomy

Scientific paper

The equation of radiative transfer is solved for spherically symmetric outflows, coupled with the equation of motion. The technique is a Legendre expansion of the spectral intensity function. The calculations, that before have been carried out for steady state only, are extended to variable mass loss rates. The results, are studied for a variety of mass loss rates variation patterns and various types of stars.

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