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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 past 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

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