Statistics – Computation
Scientific paper
Mar 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...256..519h&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 256, no. 2, p. 519-524.
Statistics
Computation
6
Radiative Transfer, Stellar Atmospheres, Stellar Rotation, Computational Astrophysics, Gravitational Effects, Opacity, Stellar Models
Scientific paper
The radiative transfer in atmosphere of a rotationally oblated star is
investigated. The horizontal diffusion of light is calculated for a gray
model in radiative equilibrium with a power law for opacity. Its
influence on the gravity darkening is discussed.
No associations
LandOfFree
Radiative transfer in rotating 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 Radiative transfer in rotating stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radiative transfer in rotating stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1214202