A more powerful evolution model for rotating stars

Details A more powerful evolution model for rotating stars A more powerful evolution model for rotating stars

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...394..965z&link_type=abstract

Astronomy and Astrophysics, v.394, p.965-969 (2002)

Astronomy and Astrophysics

Astrophysics

1

Stars: Evolution, Stars: Rotation, Stars: Hertzsprung-Russell (Hr) And C-M Diagrams

Scientific paper

A new one-dimensional rotating stellar evolution model was developed which, distinct from its previous counterparts based on a conservative rotation case or a ``shellular rotation'' case, made no special assumptions on the distribution of angular velocity inside a rotating star. The results of the evolutionary calculations are presented and compared with the results of previous studies.

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