Photometric observation and analysis of the close binary system BO Pegasi

Details Photometric observation and analysis of the close binary system BO Pegasi Photometric observation and analysis of the close binary system BO Pegasi

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98.1325y&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Dec. 1986, p. 1325-1328.

Other

4

Eclipsing Binary Stars, Light Curve, Orbital Elements, Stellar Spectrophotometry, Visual Photometry, Electrophotometry, Stellar Orbits, Ubv Spectra

Scientific paper

Photoelectric BV light curves of the close binary system BO Peg (P = 0d.580) are obtained and analyzed with a synthesis method to determine the photometric elements. It is found that the components of BO Peg are not in contact with each other but almost fill their respective Roche lobes. Two spectrograms of the system (A7 IV-V) have also been obtained, and a brief discussion on physical quantities of the components is made.

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