Theoretical evolution sequences for homogeneous and two-zone models of Delta Scuti variables

Details Theoretical evolution sequences for homogeneous and two-zone models of Delta Scuti variables Theoretical evolution sequences for homogeneous and two-zone models of Delta Scuti variables

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ssrv...27..381a&link_type=abstract

(International Astronomical Union, Colloquium on Stellar Hydrodynamics, 58th, Los Alamos, N. Mex., Aug. 12-15, 1980.) Space Scie

Astronomy and Astrophysics

Astronomy

Cepheid Variables, Pulsed Radiation, Stellar Envelopes, Stellar Evolution, Stellar Models, Helium, Resonance, Stellar Temperature

Scientific paper

Radial pulsation periods are calculated for models of variables in the lower Cepheid instability strip. Evolution tracks in several diagrams are constructed and used for comparisons with observed periods, period ratios, and effective temperatures. These comparisons are simpler and more direct than in earlier studies with separate evolution and pulsation calculations.

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