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

Investor logo
Investor logo
Investor logo

Warning

This publication doesn't include Faculty of Economics and Administration. It includes Faculty of Science. Official publication website can be found on muni.cz.
Authors

KRTIČKA Jiří MIKULÁŠEK Zdeněk ZVERKO Juraj ŽIŽŇOVSKÝ Jozef

Year of publication 2005
Type Article in Proceedings
Conference Proceedings of the IAUS224: The A-Star Puzzle
MU Faculty or unit

Faculty of Science

Citation
Web http://journals.cambridge.org/bin/bladerunner?REQUNIQ=1109866025&REQSESS=2521642&118000REQEVENT=&REQINT1=280796&REQAUTH=0
Field Astronomy and astrophysics
Keywords radiative transfer; stars: atmospheres; stars: chemically peculiar; stars: early-type
Description We calculate energy distribution of A-star atmospheres (T_eff=10 000 K, log g=4.0) for large interval of abundances of silicon and other lighter chemical elements using adequate model atmospheres. We discuss the reasons and magnitudes of found departures of the stellar energy distribution and uvby magnitudes from the normal state.
Related projects:

You are running an old browser version. We recommend updating your browser to its latest version.