Abstract Stellar seismology is a very promissing tool for the study of the stellar interior, as proven by the solar case. With high quality homogeneous data, like those obtained by multi-site photometric networks, several modes can be detected in large amplitude pulsators. They permit to extend the seimology techniques to stars. The first results of the multi-sites photometric STEPHI program are presented and a few astrophysical implications are sketched.
Stephi-seismology of δ scuti stars from multi-site photometry campaigns
Advances in Space Research ; 11 , 4 ; 167-170
1991-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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