Volume 411, Number 3, December I 2003
|Page(s)||483 - 487|
|Section||Stellar structure and evolution|
|Published online||17 November 2003|
Curious Variables Experiment (CURVE) CCD photometry of QW Serpentis in superoutburst and quiescence
Nicolaus Copernicus Astronomical Center, ul. Bartycka 18, 00-716 Warszawa, Poland
2 Warsaw University Observatory, Al. Ujazdowskie 4, 00-478 Warszawa, Poland e-mail: (pkedzier,kzlocz,kmularcz,mwisniew)@astrouw.edu.pl
Corresponding author: A. Olech, firstname.lastname@example.org
Accepted: 8 August 2003
We report extensive photometry of the dwarf nova QW Ser throughout its February 2003 superoutburst untill quiescence. During the superoutburst the star displayed clear superhumps with a mean period of days. In the quiescence we observed a double humped wave characterized by a period of days. As both periods obey the Stolz-Schoembs relation with a period excess equal to %, the latter period is interpreted as the orbital period of the binary system
Key words: stars: individual: QW Ser / stars: binaries: close / stars: novae, cataclysmic variables
© ESO, 2003
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