SIMBAD references

2016MNRAS.457.4330Y - Mon. Not. R. Astron. Soc., 457, 4330-4339 (2016/April-3)

Stability analysis, non-linear pulsations and mass loss of models for 55 Cygni (HD 198478).

YADAV A.P. and GLATZEL W.

Abstract (from CDS):

55 Cygni is a variable supergiant. Recent observational studies revealed that this star pulsates in pressure, gravity and strange modes. The pulsations seem to be associated with episodes of mass loss. In this paper we present a theoretical study of stellar models with parameters close to that of 55 Cygni. A linear non-adiabatic stability analysis with respect to radial perturbations is performed and the evolution of instabilities into the non-linear regime is followed by numerical simulation. Our study indicates that the mass of 55 Cygni lies below 28 M. As the final consequence of the instabilities the non-linear simulations revealed finite amplitude pulsations with periods consistent with the observations. The non-linear results also indicate a connection between pulsations and mass loss and allow for an estimate of the mean mass-loss rate. It is consistent with the observed values.

Abstract Copyright: © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): stars: massive - stars: mass-loss - stars: oscillations - supergiants - stars: winds, outflows

Simbad objects: 3

goto Full paper

goto View the reference in ADS

To bookmark this query, right click on this link: simbad:2016MNRAS.457.4330Y and select 'bookmark this link' or equivalent in the popup menu


2020.09.30-21:53:30

© Université de Strasbourg/CNRS

    • Contact