The dependence of the energy distribution on the abundances of A-star atmosphere models

Details The dependence of the energy distribution on the abundances of A-star atmosphere models The dependence of the energy distribution on the abundances of A-star atmosphere models

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..224..706k&link_type=abstract

The A-Star Puzzle, held in Poprad, Slovakia, July 8-13, 2004. Edited by J. Zverko, J. Ziznovsky, S.J. Adelman, and W.W. Weiss,

Other

2

Radiative Transfer, Stars: Atmospheres, Stars: Chemically Peculiar, Stars: Early-Type.

Scientific paper

We calculated the energy distributions of A-star atmospheres ({Teff=10 000} K,{log g=4.0}) for ranges of the abundances of silicon and other light chemical elements using adequate model atmospheres. We discuss the reasons for and the magnitudes of the calculated departures of the stellar energy distribution and uvby magnitudes from those of normal stars.

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