Results 11 to 20 of about 210,797 (284)
Photometric Solutions for Detached Eclipsing Binaries: selection of ideal distance indicators in the SMC [PDF]
, 2001 Detached eclipsing binary stars provide a robust one-step distance determination to nearby galaxies. As a by-product of Galactic microlensing searches, catalogs of thousands of variable stars including eclipsing binaries have been produced by the OGLE, MACHO and EROS collaborations.
Barnes T. G. +10 more
arxiv +4 more sources
KEPLERECLIPSING BINARY STARS. II. 2165 ECLIPSING BINARIES IN THE SECOND DATA RELEASE [PDF]
The Astronomical Journal, 2011 The Kepler Mission provides nearly continuous monitoring of ~156 000 objects with unprecedented photometric precision. Coincident with the first data release, we presented a catalog of 1879 eclipsing binary systems identified within the 115 square degree Kepler FOV. Here, we provide an updated catalog augmented with the second Kepler data release which
Robert W. Slawson +23 more
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Eclipsing Binary Stars in Open Clusters
, 2006 6 pages, 4 figures, proceedings of the conference Close Binaries in the 21st Century (Syros, Greece, June 2005), to appear in Ap ...
J. Southworth, J V Clausen
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The effect of star-spots on eclipse timings of binary stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2004 7 pages, 9 figures, accepted for publication in ...
C. A. Watson, V. S. Dhillon
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Photometric analysis of eclipsing binary stars
Iraqi Journal of Physics, 2019 In this paper, photometric analysis of two short period group of the eclipsing binaries (RS CVn); RT And and BH Vir is presented. New physical and geometric parameters were obtained by performing two computer modeling.
Bushra Qassim AL-Abudi
doaj +3 more sources
Phemenological Modeling of Eclipsing Binary Stars
, 2016 We review the method NAV (New Algol Variable) first introduced in 2012Ap.....55..536A, which uses the locally-dependent shapes of eclipses in an addition to the trigonometric polynomial of the second order (which typically describes the "out-of-eclipse" part of the light curve with effects of reflection, ellipticity and O'Connell).
И. Л. Андронов +2 more
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A Reflection Model for Eclipsing Binary Stars [PDF]
Monthly Notices of the Royal Astronomical Society, 1973 A highly accurate reflection model has been developed which emphasizes efficiency of computer calculation. It is assumed that the heating of the irradiated star must depend upon the following properties of the irradiating star: (1) effective temperature; (2) apparent area as seen from a point on the surface of the irradiated star; (3) limb darkening ...
D. B. Wood
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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
doaj +4 more sources
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
doaj +2 more sources
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