Line blanketed model atmospheres of AP stars. III - Alpha square Canum Venaticorum

Details Line blanketed model atmospheres of AP stars. III - Alpha square Canum Venaticorum Line blanketed model atmospheres of AP stars. III - Alpha square Canum Venaticorum

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....86..240m&link_type=abstract

Astronomy and Astrophysics, vol. 86, no. 1-2, June 1980, p. 240-244. Research supported by the Oesterreichischer Fonds zur Foer

Astronomy and Astrophysics

Astrophysics

22

A Stars, Atmospheric Models, Stellar Atmospheres, Stellar Spectrophotometry, Ultraviolet Spectra, Chemical Composition, Spectral Energy Distribution, Stellar Gravitation, Stellar Structure, Stellar Temperature, Turbulence

Scientific paper

Line blanketed model atmospheres were fitted to the absolute UV photometry and visual scans of alpha square CVn at phases 0.0 and 0.5 of the rotation period, using the chemical compositions appropriate for the corresponding phases. The results show that iron is the dominant element influencing the energy distribution of the emergent flux. The fit of models to observations suggests alpha square CVn to be hotter in phase 0.5 by about 500 K.

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