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]
Eric L. Sandquist+15 more
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Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries
Starting from more than 11,200 short-period (less than 0.5 days) EW-type eclipsing binary candidates with the All-Sky Automated Survey for Supernovae V -band light curves, we use the Markov Chain Monte Carlo algorithm and neural networks to obtain the ...
Xu-Zhi Li+6 more
doaj +1 more source
Phenomenological modeling of the light curves of algol-type eclipsing binary stars [PDF]
И. Л. Андронов
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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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Identifying stars of mass >150 M⊙ from their eclipse by a binary companion [PDF]
Tony Pan, Abraham Loeb
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TYC 3340-2437-1: A Quadruple System with a Massive Star
Hierarchical massive quadruple systems are ideal laboratories for examining the theories of star formation, dynamical evolution, and stellar evolution.
Jiao Li+13 more
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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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With the continuous development of large optical surveys, a large number of light curves of late-type contact binary systems (CBs) have been released.
JinLiang Wang+5 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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