Photometric study of AE Phoenicis

Details Photometric study of AE Phoenicis Photometric study of AE Phoenicis

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975aj.....80..140w&link_type=abstract

Astronomical Journal, vol. 80, Feb. 1975, p. 140-144.

Astronomy and Astrophysics

Astronomy

14

Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Ubv Spectra, Eccentric Orbits, Optical Filters, Tables (Data), Ultraviolet Spectra, Variable Stars

Scientific paper

The bright W Ursae Majoris-type eclipsing binary system AE Phoenicis was observed with UBV filters during 1970 at the Cerro Tololo Inter-American Observatory. A significant asymmetry in maximum light was observed and evidence for a small orbital eccentricity was detected. The eclipses are complete, and solutions of the light curves based on the Russell method give k equals 0.57.

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