The Combination Instability in Pulsating Models of Rotating Stellar Systems

Details The Combination Instability in Pulsating Models of Rotating Stellar Systems The Combination Instability in Pulsating Models of Rotating Stellar Systems

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1531....5n&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1531/SEPT, P.5 , 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

It is shown that for a certain value of the rotation angular velocity of
a pulsating system the combination of two frequencies of collective
motions coincides with the oscillation frequency of individual stars and
a new type of instability arises in the system.

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