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
Kepler Eclipsing Binary Stars. IV. Precise Eclipse Times for Close Binaries and Identification of Candidate Three-Body Systems [PDF]
, 2013 We present a catalog of precise eclipse times and analysis of third body signals among 1279 close binaries in the latest Kepler Eclipsing Binary Catalog. For these short period binaries, Kepler's 30 minute exposure time causes significant smearing of light curves.
K. Conroy +5 more
arxiv +3 more sources
KEPLERECLIPSING BINARY STARS. II. 2165 ECLIPSING BINARIES IN THE SECOND DATA RELEASE [PDF]
, 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 deg2 Kepler ...
Robert W. Slawson +23 more
openalex +3 more sources
Magnetic Inflation and Stellar Mass. I. Revised Parameters for the Component Stars of the Kepler Low-mass Eclipsing Binary T-Cyg1-12664 [PDF]
, 2017 Several low-mass eclipsing binary stars show larger than expected radii for their measured mass, metallicity, and age. One proposed mechanism for this radius inflation involves inhibited internal convection and starspots caused by strong magnetic fields.
Eunkyu Han +8 more
openalex +3 more sources
Discovery and Precise Characterization by the MEarth Project of LP 661-13, an Eclipsing Binary Consisting of Two Fully Convective Low-mass Stars [PDF]
, 2017 We report the detection of stellar eclipses in the LP 661-13 system. We present the discovery and characterization of this system, including high-resolution spectroscopic radial velocities and a photometric solution spanning two observing seasons. LP 661-
Jason Dittmann +9 more
openalex +3 more sources
Phenomenological modeling of the light curves of algol-type eclipsing binary stars [PDF]
, 2012 We propose a special class of functions for mathematical modeling of periodic signals of a special type with a nonuniform distribution of the arguments.
И. Л. Андронов
openalex +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
Modelling of W UMa-type variable stars
South African Journal of Science, 2010 W Ursae Majoris (W UMa)-type variable stars are over-contact eclipsing binary stars. To understand how these systems form and evolve requires observations spanning many years, followed by detailed models of as many of them as possible.
P. Skelton, D. Smits
doaj +13 more sources
Physical parameters of 62 eclipsing binary stars using the All Sky Automated Survey-3 data − I [PDF]
, 2011 We present a detailed light curve analysis of publicly available V band observations of 62 binary stars, mostly contact binaries, obtained by the All Sky Automated Survey (ASAS)-3 project between 2000 and 2009.
Sukanta Deb, Harinder P. Singh
openalex +3 more sources
TESS Eclipsing Binary Stars. I. Short-cadence Observations of 4584 Eclipsing Binaries in Sectors 1–26 [PDF]
Astrophysical Journal Supplement Series, 2021 In this paper we present a catalog of 4584 eclipsing binaries observed during the first two years (26 sectors) of the TESS survey. We discuss selection criteria for eclipsing binary candidates, detection of hitherto unknown eclipsing systems ...
A. Prša +46 more
semanticscholar +1 more source