Times of Minima of Eight Eclipsing Binaries

Details Times of Minima of Eight Eclipsing Binaries Times of Minima of Eight Eclipsing Binaries

May 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ibvs.4194....1i&link_type=abstract

Information Bulletin on Variable Stars, 4194, 1.

Computer Science

2

Scientific paper

We report times of minima of eccentric eclipsing binaries derived from photometric observations made at Ege University Observatory in Turkey and at Cerro Tololo Interamerican Observatory (CTIO) in Johnson B and V filters, and at the High Altitude Maidanak Observatory in Uzbekistan in Johnson U,B,V,R filters. Heliocentric times of minimum were estimated for each filter by using the method of Kwee and Van Woerden (1956) as adapted to a Macintosh computer. The adopted time of minimum was then the average over all filters. In all cases the times of minimum in different filters was concordant. Uncertainties in the times of minima were estimated from the values of standard error computed by the method and from the differences in times derived from the various filters used. Primary eclipses are designated as type 1 eclipses, and secondary eclipses as type 2.

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