Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-05-03
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
ApJ accepted
Scientific paper
Zero age main sequence models of uniformly rotating stars have been computed for ten masses between 1.625 and 8 M_\odot and 21 rotation rates from zero to nearly critical rotation. The surface shape is used to distinguish rotation rather than the surface equatorial velocity or the rotation rate. Using the surface shape is close to, but not quite equivalent to using the ratio of the rotation rate to the critical rotation rate. Using constant shape as the rotation variable means that it and the mass are separable, something that is not true for either the rotation rate or surface equatorial velocity. Thus a number of properties, including the ratio of the effective temperature anywhere on the surface to the equatorial temperature, are nearly independent of the mass of the model, as long as the rotation rate changes in such a way to keep the surface shape constant.
No associations
LandOfFree
Structure of Uniformly 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 Structure of Uniformly Rotating Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of Uniformly Rotating Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-693879