Results 221 to 230 of about 1,270 (239)
Fundamental effective temperature measurements for eclipsing binary stars – II. The detached F-type eclipsing binary CPD-54 810 [PDF]
Monthly Notices of the Royal Astronomical Society, 2022 CPD-54 810 is a double-lined detached eclipsing binary containing two mid-F type dwarfs on an eccentric 26-d orbit. We perform a combined analysis of the extensive photometry obtained by the TESS space mission along with previously published observations
N J Miller +2 more
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The origin and evolution of magnetic white dwarfs in close binary stars [PDF]
Nature Astronomy, 2021 The origin of magnetic fields in white dwarfs remains a fundamental unresolved problem in stellar astrophysics. In particular, the very different fractions of strongly (more than about a megagauss) magnetic white dwarfs in evolutionarily linked ...
M R Schreiber +2 more
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The Evolutionary Statuses of Solar Type Detached Eclipsing Binary Stars
Journal of Astronomy and Space Sciences, 2012 We presented fundamental stellar parameters and evolutionary statuses of six solar type detached eclipsing binaries whose masses are in the range of 0.97-1.43 M⊙. EK Cep and FL Lyr belong to the zero age main sequence.
Sungeun Kim +5 more
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ellc: A fast, flexible light curve model for detached eclipsing binary stars and transiting exoplanets [PDF]
Astronomy and Astrophysics, 2016 Very high quality light curves are now available for thousands of detached eclipsing binary stars and transiting exoplanet systems as a result of surveys for transiting exoplanets and other large-scale photometric surveys.
P F L Maxted
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Investigation of near-contact semi-detached binary WUMi through observations and evolutionary models [PDF]
Research in Astronomy and Astrophysics, 2020 W UMi is a near contact, semi-detached, double-lined eclipsing binary star with an orbital period of 1.7 d. Simultaneous analysis of new BV R multi-color light curves and radial velocity data yields the main astrophysical parameters of the binary and its
F Soydugan, Fahri Aliçavus
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Automatic classification of eclipsing binary stars using deep learning methods
Astronomy and Computing, 2021Viera Maslej-Krešňáková +2 more
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Gravity-darkening exponents in semi-detached binary systems from their photometric observations. II.
Astronomy and Astrophysics, 2006G Djurasevic +2 more
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Photometric Mass Ratios of Eclipsing Binary Stars
Astrophysics and Space Science, 2005Dirk Terrell, R E Wilson, Wilson R E
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