Mode identification in Beta Cephei stars

Details Mode identification in Beta Cephei stars Mode identification in Beta Cephei stars

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980cpsp.book..331a&link_type=abstract

In its Current Probl. in Stellar Pulsation Instabilities p 331-361 (SEE N80-25229 15-90)

Computer Science

1

Cepheus Constellation, Radial Velocity, Stellar Spectra, Variable Stars, Angular Velocity, Graphs (Charts), Line Spectra, Stellar Luminosity

Scientific paper

The essential observational characteristics related to mode identification are summarized. Major emphasis is placed on the following: both light and velocity amplitudes; typical periods in both light and radial velocity; the light curve for Beta Cephei stars in comparison to the classical Cepheids and RR Lyrae stars; the van Hoof effect with respect to the radial velocity curves in many Beta Cephei stars; and the line profiles of many Beta Cephei stars.

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