The theoretical red edge of the RR Lyrae gap. III - Overtone pulsation

Details The theoretical red edge of the RR Lyrae gap. III - Overtone pulsation The theoretical red edge of the RR Lyrae gap. III - Overtone pulsation

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...215..232d&link_type=abstract

Astrophysical Journal, Part 1, vol. 215, July 1, 1977, p. 232-235. ERDA-supported research.

Astronomy and Astrophysics

Astrophysics

30

Giant Stars, Stellar Models, Stellar Structure, Convective Flow, Hertzsprung-Russell Diagram, Hydrogen, Modal Response

Scientific paper

The theoretical location of the red edge of the RR Lyrae gap is found
for models pulsating in the first overtone mode. Convection causes a
return to pulsational stability for these models. The location of the
red edge for the overtone models is to the blue of the red edge for
fundamental mode pulsators.

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