Physical parameters of 62 eclipsing binaries (Deb+, 2011)

Details Physical parameters of 62 eclipsing binaries (Deb+, 2011) Physical parameters of 62 eclipsing binaries (Deb+, 2011)

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74121787d&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/412/1787. Originally published in: 2011MNRAS.412.1787D

Astronomy and Astrophysics

Astronomy

Binaries: Eclipsing, Photometry, Morphology, Stars: Masses

Scientific paper

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. Eclipsing binaries are important astronomical targets for determining the physical parameters of component stars from the geometry of their orbits. They provide an independent direct method of measuring the radii of stars. We improved the ASAS determined periods and ephemerides, and obtained the Fourier parameters from the phased light curves of these 62 stars.
(5 data files).

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