Pulsations of luminous intermediate-mass stars with applications to UU Herculis

Details Pulsations of luminous intermediate-mass stars with applications to UU Herculis Pulsations of luminous intermediate-mass stars with applications to UU Herculis

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasp..107..238a&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 107, no. 709, p. 238-243

Astronomy and Astrophysics

Astronomy

3

F Stars, Stellar Evolution, Stellar Luminosity, Stellar Models, Stellar Oscillations, Supergiant Stars, Variable Stars, Data Correlation, Hydrodynamics, Radiative Transfer, Stellar Interiors

Scientific paper

Pulsation models for the enigmatic F-type supergiant variable, UU Herculis are investigated. It is shown that irregular pulsations with small amplitude is realized, if UU Her is assumed to be an intermediate-mass-F-type supergiant star which has evolved with mass loss and rotational mixing and thus highly luminous, compared with what is obtained by conventional evolution.

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