Physics
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358..188h&link_type=abstract
In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 188-198 (SEE N85-17755 08-88)
Physics
Heating, Magnetohydrodynamic Stability, Stellar Winds, Emission, Magnetohydrodynamics, Momentum, Stellar Mass Ejection, Stellar Structure, Stellar Temperature, Supersonic Flow, X Rays
Scientific paper
The mass loss and acceleration of the mass flow comes, directly or indirectly, from the radiative forces of the resonance lines. These radiative forces can also cause instabilities to grow in the flow, and this is probably an important source of non-radiative heating and momentum in hot stars. The physical origin of these instabilities is described, and some of the problems of hot stars where radiative driven instabilities may play a part are briefly discussed.
No associations
LandOfFree
Radiatively driven winds and what they imply: A review of radiative driven instabilities and their importance in hot stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Radiatively driven winds and what they imply: A review of radiative driven instabilities and their importance in hot stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiatively driven winds and what they imply: A review of radiative driven instabilities and their importance in hot stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-927340