Results 11 to 20 of about 997,063 (252)
The Astrophysical Journal, 2023 The first detailed photometric and spectroscopic study of G-type short-period binary NY Boo is presented. The radial velocity curve was obtained by the cross-correlation function (CCF) method based on LAMOST and SDSS spectra, which derived its mass ratio
Fangbin Meng +5 more
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V772 Cas: an ellipsoidal HgMn star in an eclipsing binary [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 ABSTRACT The late B-type star V772 Cas (HD 10260) was previously suspected to be a rare example of a magnetic chemically peculiar star in an eclipsing binary system. Photometric observations of this star obtained by the TESS satellite show clear eclipses with a period of 5.0137 d accompanied by a significant out-of-eclipse variation with
O. Kochukhov +6 more
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Discovery and characterisation of long-period eclipsing binary stars from Kepler K2 campaigns 1, 2 and 3 [PDF]
, 2018 The Kepler K2 mission now makes it possible to find and study a wider variety of eclipsing binary stars than has been possible to-date, particularly long-period systems with narrow eclipses.
Maxted
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Mass-Accreting Pulsating Components of Algols
Galaxies, 2022 We present a review of the latest results of studies of the class of mass-accreting pulsating components of semi-detached eclipsing binaries known as oEA stars.
David Mkrtichian +5 more
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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 ...
Watson, C. A., Dhillon, V. S.
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Eclipsing Binaries in Multiple Star Systems [PDF]
Symposium - International Astronomical Union, 1992 Although the majority of the known eclipsing binaries are in systems which consist of only the two eclipsing components, a significant number of them do occur as components of triple star systems or higher order multiple star systems. In this context this term is restricted to those systems whose components are in closed orbits.
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A catalogue of temperatures for Kepler eclipsing binary stars [PDF]
Monthly Notices of the Royal Astronomical Society, 2013 We have combined the Kepler Eclipsing Binary Catalogue with information from the HES, KIS and 2MASS photometric surveys to produce spectral energy distribution fits to over 2600 eclipsing binaries in the catalogue over a wavelength range of 0.36 to 2.16Å.
Armstrong, D. J. +3 more
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A Search for Exoplanets in Short-Period Binary Star Systems [PDF]
Journal of Astronomy and Space Sciences, 2012 This paper reports the progress of a search for exoplanets with S-type orbits in short-period binary star systems. The selected targets have stellar orbital periods of just a few days. These systems are eclipsing binaries so that exoplanet transits, if
Ronald Kaitchuck +2 more
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Eclipsing binaries observed with the WIRE satellite. II, β Aurigae and non-linear limb darkening in light curves [PDF]
, 2007 Aims. We present the most precise light curve ever obtained of a detached eclipsing binary star and use it investigate the inclusion of non-linear limb darkening laws in light curve models of eclipsing binaries.
Southworth, J. (John) +5 more
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Infrared photometry of eclipsing binary stars.
, 1978 The infrared observations of several eclipsing binary stars are presented and discussed. Initially a brief review of the relevant literature is given together with a description of binary systems, in particular eclipsing binary stars. This is followed by
R. Akinci (7699997)
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