A photometric orbit for the eclipsing binary AG Phoenicis

Details A photometric orbit for the eclipsing binary AG Phoenicis A photometric orbit for the eclipsing binary AG Phoenicis

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pasp...95..347c&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 95, June 1983, p. 347-353.

Astronomy and Astrophysics

Astronomy

1

Eclipsing Binary Stars, Orbital Elements, Stellar Spectrophotometry, Light Curve, Stellar Color, Ubv Spectra

Scientific paper

In each of the UBV bandpasses about 1760 observations define for the
first time the photoelectric light variation of the binary system AG
Phe. A consistent set of elements is derived in the framework of the
classical model. The system would be a well-detached binary consisting
of two normal A9 and K0 main-sequence components.

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