Simultaneous UVBY beta photometry of SX Phoenicis stars

Details Simultaneous UVBY beta photometry of SX Phoenicis stars Simultaneous UVBY beta photometry of SX Phoenicis stars

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as..100..571r&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 100, no. 3, p. 571-581.

Astronomy and Astrophysics

Astrophysics

11

Astronomical Photometry, Light Curve, Variable Stars, Space Observations (From Earth), Stellar Evolution

Scientific paper

In this paper, we present simultaneous uvby beta photometric observations of five SX Phe stars: XX Cyg, CY Aqr, DY Peg, BS Tuc, and SU Crt. The light curves were obtained at Sierra Nevada Observatory, Granada, Spain and European Southern Observatory, La Silla, Chile on 30 nights from 1986 through 1988 and contain 847 points in each of the four uvby colors of the Stromgren photometric system and 542 points in each of the two narrow and wide channels of the H-beta Crawford system.

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