Ref HAL: hal-01966612_v1
DOI: 10.1051/0004-6361/201322794
Exporter : BibTex | endNote
11 citations

DOI: 10.1007/s10511-014-9354-5
4 citations
Résumé:

The goal of this paper is to present an optical variability study of the comparatively faint carbon (C) stars which have been discovered by searching the First Byurakan Survey (FBS) low-resolution (lr) spectral plates at high Galactic latitudes using recent wide-area variability databases. The light curves from the Catalina Sky Survey (CSS) and Northern Sky Variability Survey (NSVS) databases were exploited to study theit variability nature. In this paper, first in this series, the variability classes are presented for 54 N-type Asymptotic Giant Branch (AGB) C stars. One finds that 9 stars belongs to the group of Mira-type, 43 are Semi-Regular (SR), and 2 stars are Irregular (Irr)-type variables. The variability types of 27 objects has been established for the first time. K-band absolute magnitudes, distances, and height from the Galactic plane were estimated for all of them. We aim to better understand the nature of the selected C stars through spectroscopy, 2MASS photometric colors, and variability data. Most of the tools used in this study are developed within the framework of the Astronomical Virtual Observatory.

Résumé:

Mass loss of red supergiants is important for the evolution of massive stars, but not fully explained. Several empirical prescriptiosn have been proposed, trying to express Mdot as a function of fundamental stellar parameters. etc