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Stellar Parameters of the Post-AGB Star HD 56126

Published online by Cambridge University Press:  12 April 2016

H. Le Coroller ,
D. Gillet ,
A.B. Fokin  and
A. Lèbre
H. Le Coroller*
Affiliation:
Observatoire de Haute-Provence (CNRS), France
D. Gillet
Affiliation:
Observatoire de Haute-Provence (CNRS), France
A.B. Fokin
Affiliation:
Institute of Astronomy, Russian Academy of Sciences, Russia
A. Lèbre
Affiliation:
GRAAL, Université Montpellier II & CNRS, France
*
1 e-mail: coroller@obs-hp.fr

Abstract

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We discuss the stellar parameters (M, L, Teff) of a post-AGB star, HD 56126, deduced from observations and non-linear radiative pulsation models. We show that pure radiative pulsation models are in contrast with stellar evolution.

Type
Part 5. Mass Loss in Pulsating Stars
Information
International Astronomical Union Colloquium , Volume 185: Radial and Nonradial Pulsations as Probes of Stellar Physics , 2002 , pp. 578 - 579
Copyright
Copyright © Astronomical Society of the Pacific 2002

References

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