The Limits of Inclination for Binary Star Partial Eclipses
Algorithms are given for calculating the inclinations at which total eclipses become partial eclipses and partial eclipses become grazing eclipses. It is shown that the larger star in a contact or nearly contact system is so distorted in shape that it becomes self-eclipsing, as a shallow concavity develops near the point of contact. Algorithms are also
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An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i. [PDF]
Kipping D+8 more
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Phenomenological modeling of the light curves of algol-type eclipsing binary stars [PDF]
И. Л. Андронов
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MG1-1995959: An Eclipsing Binary Star with a Pronounced O’Connell Effect
MG1-1995959 is a short-period (∼0.586 day) eclipsing binary, exhibiting at times an extraordinarily large O’Connell effect (OE), for which this paper reports its discovery, time series photometry, and spectroscopic observation.
Eric R. Craine+10 more
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Orbital period change of Dimorphos due to the DART kinetic impact. [PDF]
Thomas CA+48 more
europepmc +1 more source
Identifying stars of mass >150 M⊙ from their eclipse by a binary companion [PDF]
Tony Pan, Abraham Loeb
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ECLIPSING BINARY STARS AS BENCHMARKS FOR TRIGONOMETRIC PARALLAXES IN THE GAIA ERA [PDF]
Keivan G. Stassun, Guillermo Torres
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This paper selected eight totally eclipsing contact binaries for photometric and spectroscopic studies. Spectral data were analyzed by University of Lyon Spectroscopic analysis Software, and photometric data were analyzed using PHOEBE through Markov ...
Li-Heng Wang+6 more
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New Pulsating Stars Detected in EA-type Eclipsing-binary Systems Based on TESS Data
Xiang-Dong Shi+2 more
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Discovery and Precise Characterization by the MEarth Project of LP 661-13, an Eclipsing Binary Consisting of Two Fully Convective Low-mass Stars [PDF]
Jason Dittmann+9 more
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