The rapidly oscillating AP stars

Details The rapidly oscillating AP stars The rapidly oscillating AP stars

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...143..206g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 143, no. 1, Feb. 1985, p. 206-208.

Astronomy and Astrophysics

Astrophysics

32

A Stars, Main Sequence Stars, Peculiar Stars, Stellar Models, Stellar Oscillations, Cool Stars, Hertzsprung-Russell Diagram, Stellar Evolution, Vibration Mode

Scientific paper

Frequency separation delta nu between consecutive modes have been
computed for rapidly oscillating stars. It is shown that delta nu is a
good indicator of the star's position in the main sequence band. These
results are applied to Kurtz (1980 and 1982) observations of HD 101065
and HD 24712. The problem of HD 83368 is also discussed.

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