Pulsating and Chemically Peculiar Upper Main Sequence Stars

Details Pulsating and Chemically Peculiar Upper Main Sequence Stars Pulsating and Chemically Peculiar Upper Main Sequence Stars

Nov 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000eaa..booke5201k&link_type=abstract

"Encyclopedia of Astronomy and Astrophysics, Edited by Paul Murdin, article 5201. Bristol: Institute of Physics Publishing, 2001

Astronomy and Astrophysics

Astrophysics

Stars, Stellar Models And Concepts

Scientific paper

There is a natural astrophysical division of the main sequence which occurs for early F stars. Stars cooler than this have deep surface convection zones, radiative cores, generate their energy by the proton-proton cycle, rotate relatively slowly and any global magnetic field present is weak, although strong fields may exist in tangled flux tubes, as in sunspots in the Sun. Stars hotter than early...

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