Radiative transfer in hydrodynamical protostar models. I - Method and preliminary results

Details Radiative transfer in hydrodynamical protostar models. I - Method and preliminary results Radiative transfer in hydrodynamical protostar models. I - Method and preliminary results

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51..101b&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 1, Aug. 1976, p. 101-105. Deutsche Forschungsgemeinschaft

Astronomy and Astrophysics

Astrophysics

12

Hydrodynamics, Protostars, Radiative Transfer, Stellar Envelopes, Stellar Evolution, Stellar Models, Computer Techniques, Extensions, Spectral Energy Distribution, Stellar Mass, T Tauri Stars, Ubv Spectra

Scientific paper

A method of solution for the nongrey radiative-transfer problem in the extended envelopes of protostars is described. This method has been coupled to the hydrodynamic evolutionary code of Appenzeller and Tscharnuter (1974, 1975). Preliminary numerical results for the evolution in spectral appearance of a one-solar-mass protostar are discussed.

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