Copyright © International Astronomical Union 2015. We study spectra of two bona fide LBV stars in M31: AF And and Var 15. The spectra were obtained with the 6-m telescope (Russia) from 2005 to 2012. The model spectra were calculated with the CMFGEN code. We have not found strong changes in the spectra of the LBV stars in that time interval, however a certain variability has been detected. We estimate the star and wind parameters, such as luminosity, temperature, raduis, mass loss rate, escape velocity, hydrogen content, and reddening. We study the stars on the Hertzsprung-Russell diagram and find their initial masses using evolutionary tracks by Meynet et al. (1994)
Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the...
Context. Understanding the origin of the instabilities of LBVs is important for shedding light on th...
We report on the binarity of luminous blue variable stars observed with a set of techniques and inst...
Copyright © International Astronomical Union 2015. We study spectra of two bona fide LBV stars in M3...
© 2015 The Authors. We performed spectroscopy of five luminous blue variable (LBV) candidates and tw...
The thesis is dealing with spectral analysis of the B[e] star FS CMa, a prototype of FS CMa stars gr...
Leuchtkräftige Blaue Veränderliche (LBVs) zeigen photometrische und spektrale Variabilität, welche a...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
International audienceContext. The evolution of massive stars depends on several parameters, and the...
B[e] stars are a peculiar group of stars with forbidden emission lines in their spectra. This phenom...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
This thesis deals with the study of the star V743 Mon. Stellar spectrum contains forbidden emission ...
We present integral field spectroscopy of the LBV candidate stars B416 and v532 in the local group g...
Aims: We present a spectroscopic analysis of MWC 314, a luminous blue variable (LBV) candidate with ...
We present the results of the analysis of 56 échelle spectra of the β Cephei star BW Vulpeculae. The...
Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the...
Context. Understanding the origin of the instabilities of LBVs is important for shedding light on th...
We report on the binarity of luminous blue variable stars observed with a set of techniques and inst...
Copyright © International Astronomical Union 2015. We study spectra of two bona fide LBV stars in M3...
© 2015 The Authors. We performed spectroscopy of five luminous blue variable (LBV) candidates and tw...
The thesis is dealing with spectral analysis of the B[e] star FS CMa, a prototype of FS CMa stars gr...
Leuchtkräftige Blaue Veränderliche (LBVs) zeigen photometrische und spektrale Variabilität, welche a...
© 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
International audienceContext. The evolution of massive stars depends on several parameters, and the...
B[e] stars are a peculiar group of stars with forbidden emission lines in their spectra. This phenom...
Context. Luminous blue variables (LBVs) are a class of highly unstable stars that have been proposed...
This thesis deals with the study of the star V743 Mon. Stellar spectrum contains forbidden emission ...
We present integral field spectroscopy of the LBV candidate stars B416 and v532 in the local group g...
Aims: We present a spectroscopic analysis of MWC 314, a luminous blue variable (LBV) candidate with ...
We present the results of the analysis of 56 échelle spectra of the β Cephei star BW Vulpeculae. The...
Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the...
Context. Understanding the origin of the instabilities of LBVs is important for shedding light on th...
We report on the binarity of luminous blue variable stars observed with a set of techniques and inst...