The ups and downs of a stellar surface: nonradial pulsation modelling of rapid rotators

Details The ups and downs of a stellar surface: nonradial pulsation modelling of rapid rotators The ups and downs of a stellar surface: nonradial pulsation modelling of rapid rotators

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002msngr.108...20r&link_type=abstract

The Messenger, No. 108, p. 20 - 24 (June 2002)

Physics

2

Stellar Surfaces, Nonradial Pulsations, Stellar Rotation

Scientific paper

The main result of the modelling project is the confirmation that
early-type Be stars pulsate nonradially in g-modes. Based on the
detailed modelling of ω CMa, it could be shown that this star is
proto-typical, and that the periodic lpv of early type Be stars in
general is due to nonradial pulsation.

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