Photometric analysis of the eclipsing binary RX Hydrae

Details Photometric analysis of the eclipsing binary RX Hydrae Photometric analysis of the eclipsing binary RX Hydrae

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26as...81...67v&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 81, no. 1, Nov. 1989, p. 67-79. Research supported by UGCI.

Astronomy and Astrophysics

Astrophysics

4

Astronomical Photometry, Early Stars, Eclipsing Binary Stars, Late Stars, Main Sequence Stars, Light Curve, Mass Transfer, Stellar Magnitude, Stellar Mass, Subgiant Stars

Scientific paper

Complete photoelectric U, B, and V light curves were obtained for the
single-lined eclipsing binary, RX Hydrae, in 1983-1987. The results
suggest that the system is a semidetached Algol-type binary in which the
secondary is filling its roche lobe. Also, results are given from a
period variation study for RX Hydrae.

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