Phenomenological modeling of the light curves of algol-type eclipsing binary stars [PDF]
, 2012 We propose a special class of functions for mathematical modeling of periodic signals of a special type with a nonuniform distribution of the arguments.
И. Л. Андронов
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Fundamental Properties of Late-Type Stars in Eclipsing Binaries
Galaxies, 2022 Evidence from the analysis of eclipsing binary systems revealed that late-type stars are larger and cooler than predicted by models, and that this is probably caused by stellar magnetic activity.
Juan Carlos Morales +3 more
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MASS TRANSFER IN ECLIPSING BINARY STARS
Odessa Astronomical Publications, 2017 Analysis of the properties of the eclipsing binary stars shows, that the stream-like mechanism of the mass transfer switches on at a contact evolutionary stage, preceding to a stage of binaries with a subgiant.
V. G. Karetnikov +2 more
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Variability in the Massive Open Cluster NGC 1817 from K2: A Rich Population of Asteroseismic Red Clump, Eclipsing Binary, and Main-sequence Pulsating Stars. [PDF]
Astron J, 2020 Sandquist EL +15 more
europepmc +3 more sources
Calculation of Eclipse Functions for Binary Stars.
The Astronomical Journal, 1964 Albert P. Linnell
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TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26 [PDF]
Astrophysical Journal Supplement Series, 2021 In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary candidates, detection of hitherto unknown eclipsing systems ...
A. Prša +46 more
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The surface brightness–colour relations based on eclipsing binary stars and calibrated with Gaia EDR3 [PDF]
Astronomy & Astrophysics, 2021 Aims. The surface brightness–colour relation (SBCR) is a basic tool for establishing precise and accurate distances within the Local Group. Detached eclipsing binary stars with accurately determined radii and trigonometric parallaxes allow calibration of
D. Graczyk +25 more
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Classification of OGLE Eclipsing Binary Stars Based on Their Morphology Type with Locally Linear Embedding [PDF]
, 2021 The Optical Gravitational Lensing Experiment (OGLE) continuously monitors hundreds of thousands of eclipsing binaries in the Galactic bulge field and the Magellanic Clouds.
A. B'odi, Tam'as Hajdu
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A Distance Determination to the Small Magellanic Cloud with an Accuracy of Better than Two Percent Based on Late-type Eclipsing Binary Stars [PDF]
Astrophysical Journal, 2020 We present a new study of late-type eclipsing binary stars in the Small Magellanic Cloud (SMC) undertaken with the aim of improving the distance determination to this important galaxy.
D. Graczyk +19 more
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Fundamental effective temperature measurements for eclipsing binary stars – I. Development of the method and application to AI Phoenicis [PDF]
Monthly notices of the Royal Astronomical Society, 2020 Stars with accurate and precise effective temperature (Teff) measurements are needed to test stellar atmosphere models and calibrate empirical methods to determine Teff.
N. Miller, P. Maxted, B. Smalley
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