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.


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    Title :

    Stephi-seismology of δ scuti stars from multi-site photometry campaigns


    Contributors:
    Michel, E. (author) / Baglin, A. (author)

    Published in:

    Advances in Space Research ; 11 , 4 ; 167-170


    Publication date :

    1991-01-01


    Size :

    4 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English



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