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NLTE Model Atmospheres with Rotation

Published online by Cambridge University Press:  26 May 2016

Daniela Korčáková and
Jiří Kubát
Daniela Korčáková
Affiliation:
Astronomický ústav AV ČR, CZ-251 65 Ondřejov, Czech RepublicÚstav teoretické fyziky a astrofyziky PřF MU, Kotlářská 2, CZ-611 37 Brno, Czech Republic
Jiří Kubát
Affiliation:
Astronomický ústav AV ČR, CZ-251 65 Ondřejov, Czech Republic

Abstract

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We present a modification of our code for calculation of NLTE model atmospheres in planar and spherical geometry to the case of rotating atmospheres. This modification enables self-consistent inclusion of the effect of rotation on the atmospheric structure.

Information

Type
Session 1 Observations of Rotating Stars
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004, pp. 25 - 26
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Gray, D. F. 1976, Observation and Analysis of Stellar Photospheres, John Wiley & Sons, New York Google Scholar
Hadrava, P., Kubat, J. 2003, in Stellar Atmosphere Modelling, Hubeny, I., Mihalas, D. & Werner, K. eds., ASP Conf. Ser., in press Google Scholar
Korčáková, D., Kubát, J. 2003a, A&A, submitted Google Scholar
Korčáková, D., Kubát, J. 2003b, in Modelling of Stellar Atmospheres, IAU Symp. 210, Piskunov, N. E., Weiss, W. W. & Gray, D. F. eds., ASP Conf. Ser., submitted Google Scholar
Kubát, J. 2003a, in Stellar Atmosphere Modelling, Hubeny, I., Mihalas, D. & Werner, K. eds., ASP Conf. Ser., in press Google Scholar
Kubát, J. 2003b, in Modelling of Stellar Atmospheres, IAU Symp. 210, Piskunov, N. E., Weiss, W. W. & Gray, D. F. eds., ASP Conf. Ser., submitted Google Scholar