New luminous blue variables in the Andromeda galaxy of the
variable stars obtained in two ormore different states, and we estimate the temperatures, reddening, radii
Modeling of Extended Atmospheres with Temperatures below 40000 K number of objects with emission spectra, such as luminous blue
variables, FeII—emission line
stars, Of
Is WD 1437-008 a cataclysmic variable? classified as a low-inclination cataclysmic
variable. © 2011 Pleiades Publishing, Ltd.
MASTER OT J172758.09+380021.5: a peculiar ER UMa-type dwarf nova, probably a missed nova in the recent pastPavlenko E.,
Kato T.,
Antonyuk K.,
Pit N.,
Keir L.,
Udovichenko S.,
Dubovský P.,
Sosnovskij A.,
Antonyuk O.,
Shimansky V.,
Gabdeev M.,
Rakhmatullaeva F.,
Kokhirova G.,
Belan S.,
Simon A.,
Baklanov A.,
Kojiguchi N.,
Godunova V. done in 2020 when the object was in quiescence. Spectra and photometry revealed that the
star is an H
Asymmetrical nebula of the M33 variable GR290 (WR/LBV) photometric
variability typical for luminous blue
variable stars. It lies inside the Wolf-Rayet region
Is WD 1437-008 a cataclysmic variable? classified as a low-inclination cataclysmic
variable. © 2011 Pleiades Publishing, Ltd.
Analysis of spectra of V471 Tau and HD 115404We analyze the chemical composition of the atmospheres of a single K-type
star HD 115404
New luminous blue variables in the Andromeda galaxy of the
variable stars obtained in two ormore different states, and we estimate the temperatures, reddening, radii
Luminous blue variable candidates in M31 Society. We study five luminous blue
variable (LBV) candidates in the Andromeda galaxy and one more (MN112
Analysis of spectra of V471 Tau and HD 115404We analyze the chemical composition of the atmospheres of a single K-type
star HD 115404