The O'Connell effect systems CX Canis Majoris, TU Crucis, AQ Monocerotis, and DQ Velorum

Details The O'Connell effect systems CX Canis Majoris, TU Crucis, AQ Monocerotis, and DQ Velorum The O'Connell effect systems CX Canis Majoris, TU Crucis, AQ Monocerotis, and DQ Velorum

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apjs...61..455m&link_type=abstract

Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 61, June 1986, p. 455-464. Research supported by the University o

Astronomy and Astrophysics

Astrophysics

5

Astronomical Photometry, Eclipsing Binary Stars, Stellar Spectra, Light Curve, Orbital Elements, Ubv Spectra

Scientific paper

UBV photometry and classification spectroscopy have been carried out for four suspected O'Connell effect systems in the southern hemisphere. Although the light curves are incomplete, they represent the first photoelectric data on these systems and reveal the degree to which the O'Connell effect is present. Phases of minima were computed for all four systems, and for previously published light curves for AQ Mon. Improved elements were derived for the latter system. Fourier representations for the four systems were also determined.

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