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The measurements of brightness of the star IRAS 17583+5150 discovered using the Odessa observatory negatives are discussed in the article. The proposed types of these stars are IRAS 17583+5150 -- type SRB (SRC).
A. P. Solonovich, I. S. Bryukhanov
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Deep multi-survey classification of variable stars [PDF]
During the last decade, a considerable amount of effort has been made to classify variable stars using different machine learning techniques. Typically, light curves are represented as vectors of statistical descriptors or features that are used to train
Carlos Aguirre, K. Pichara, I. Becker
semanticscholar +1 more source
OBSERVATIONS OF VARIABLE STARS WITH SMALL TELESCOPES
No ...
I. S. Bryukhanov
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Outbursts of luminous blue variable stars from variations in the helium opacity [PDF]
Luminous blue variables are massive, evolved stars that exhibit large variations in luminosity and size on timescales from months to years, with high associated rates of mass loss1–5. In addition to this on-going variability, these stars exhibit outburst
Yan-Fei Jiang+5 more
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Measurements of brightness of stars 1AL Ari, FM Leo, LL Aqr, V1125 Tau, V1366 Ori opened in ”HIPPARCOS” experiment are carried out using negatives of the Odessa observatory.
A. P. Solonovich+2 more
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Measurements of brightness of stars TX Crv, DP Cam, IRAS 17583+5150 opened in "IRAS" and "HIPPARCOS" experiments are carried out using negatives of the Odessa observatory.
A. P. Solonovich+2 more
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Gaia Data Release 2: Variable stars in the colour-absolute magnitude diagram [PDF]
The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ~ 21 mag. We showcase stellar variability across the Galactic colour-absolute magnitude diagram (CaMD), focusing on pulsating, eruptive, and cataclysmic ...
L. Eyer+134 more
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A recurrent neural network for classification of unevenly sampled variable stars [PDF]
Astronomical surveys of celestial sources produce streams of noisy time series measuring flux versus time (‘light curves’). Unlike in many other physical domains, however, large (and source-specific) temporal gaps in data arise naturally due to ...
Brett Naul+3 more
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THE INVESTIGATION OF THE CLASSICAL CEPHEID RT Aur PERIOD
The outcomes of the research into RT Aur period for the last 93 years are given in the article. New elements of changes in RT Aur brightness have been determined by the authors: J.D.max=2447890,265+3.7283116*E.
A. S. Kosinsky+5 more
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