Night Thoughts on Slowly Variable F-Type stars

Details Night Thoughts on Slowly Variable F-Type stars Night Thoughts on Slowly Variable F-Type stars

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996dssn...10...13g&link_type=abstract

Delta Scuti Star Newsletter, Issue 10, p. 13

Physics

6

Scientific paper

This contribution is to be understood as an answer to the article of K. Krisciunas which appeared in the DSN issue 9 (1995) on the slow F-type variables - or Gamma Dor stars as they appear to be termed now. We aim at correcting the statement by Krisciunas on the number of unstable oscillation modes which were allegedly found in F-type star models by one of us (A.G.); actually we would be quite happy if this would be the case. Krisciunas must have misinterpreted estimates on the number of modes A.G. expected to be unstable if a classical destabilization mechanism were at work in the Gamma Dor stars. This occurred during a series of e-mail discussions with K.Krisciunas on the particular topic. In addition, we will contribute a few thoughts on the Gamma Dor-type variability mainly as a continuation of aspects which were touched upon in the Krisciunas article.

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