Photoelectric Minima of Some Ecliptic Binaries

Details Photoelectric Minima of Some Ecliptic Binaries Photoelectric Minima of Some Ecliptic Binaries

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004bssci.121...10y&link_type=abstract

BAA-Variable Star Section Circular, #121, p. 10-11

Physics

Eclipsing Binaries, Minima Times

Scientific paper

These binary stars were observed as a part of a project given to TUBITAK (The Scientific and Technical Research Council of Turkey) National Observatory (TUG). Some of the stars, such as V2150 Cyg and OU Ser, need much more data for both reliable O-C analysis, and defining the physical nature of these systems. The observations were performed in the Johnson V band, and reduction of the observations was made in the usual way (Hardie 1962). The standard error is included in each of the minimum times. The observations were reduced by using the method of Kwee and van Woerden (1956).

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