Morphology of a group of variable stars of the type Is(A). III - Analysis of hydrogen line profiles from high-resolution spectra

Details Morphology of a group of variable stars of the type Is(A). III - Analysis of hydrogen line profiles from high-resolution spectra Morphology of a group of variable stars of the type Is(A). III - Analysis of hydrogen line profiles from high-resolution spectra

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...71k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, no. 2, Mar.-Apr. 1992, p. 71-79. In Russian.

Physics

5

H Beta Line, H Gamma Line, High Resolution, Line Shape, Variable Stars, Main Sequence Stars, Stellar Luminosity, Stellar Models, Stellar Spectrophotometry

Scientific paper

The hydrogen line profiles of nine variable stars and 2 reference stars
were investigated using echelle spectra obtained with a 6-m telescope.
The lg g values are determined using the Kurucz model atmospheres. It is
shown that the stars investigated fall outside the main sequence on the
(lg Teff, lg g) diagram.

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