Radiative stellar winds

Details Radiative stellar winds Radiative stellar winds

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..191p&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, Apr.-May 1980, p. 191-194. NSF-supported research.

Astronomy and Astrophysics

Astronomy

1

Radiative Heat Transfer, Stellar Mass Ejection, Stellar Winds, T Tauri Stars, Transonic Flow, Cooling, Stellar Envelopes, Wind Velocity, X Ray Sources

Scientific paper

The effect of the radiative cooling on the steady-state transonic wind
model is calculated. It happens that there exists a maximum limit to the
mass-loss rate such that if the limit is exceeded, the wind will no
longer be in the steady state and turbulence may occur, giving rise to a
possible source of X rays in T Tauri objects.

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