SIMBAD references

2002A&A...385..563D - Astronomy and Astrophysics, volume 385, 563-571 (2002/4-2)

Influence of non-adiabatic temperature variations on line profile variations of slowly rotating β Cep stars and SPBs. I. Non-adiabatic eigenfunctions in the atmosphere of a pulsating star.

DUPRET M.-A., DE RIDDER J., NEUFORGE C., AERTS C. and SCUFLAIRE R.

Abstract (from CDS):

In this study, we compute theoretical line profiles of a non-radially pulsating star, taking the non-adiabatic effects into account. These non-adiabatic effects are especially important in the atmosphere, where the spectral lines are formed, and must be accounted for. In this first paper of the series, we present a new treatment of the perturbed thermal and dynamical equations in the atmosphere of a pulsating star. We apply our formalism to the computation of non-adiabatic eigenfunctions in a typical β Cephei star with low order p-modes and in a typical slowly pulsating B star with high-order g-modes.

Abstract Copyright:

Journal keyword(s): stars: oscillations - stars: atmospheres - line: profiles - stars: variables: β Cep - stars: variables: slowly fulsating B stars

Simbad objects: 1

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2002A&A...385..563D and select 'bookmark this link' or equivalent in the popup menu


2019.10.24-02:40:57

© Université de Strasbourg/CNRS

    • Contact