Multi-site observation of the δ Scuti star V 647 Tau. Primary results of the Eighth STEPHI campaign

Details Multi-site observation of the δ Scuti star V 647 Tau. Primary results of the Eighth STEPHI campaign Multi-site observation of the δ Scuti star V 647 Tau. Primary results of the Eighth STEPHI campaign

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cha%26a..23..349l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 23, Issue 3, p. 349-360.

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The eighth STEPHI international multi-site campaign was devoted to the δ Scuti Star V647 Tau of the Pleiades Cluster and was carried out in the period 1997 Nov 19-Dec 13. Analysis using two methods gave the same result. Five pulsation frequencies including both radial and non-radial modes are excited in this star. The dominant frequency p = 20.408c/d observed in 1972 has decreased to become the second frequency with a decreased amplitude. The global parameters show the star to be a young A type star just beginning core hydrogen burning.

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