SIMBAD references

2003A&A...411..483O - Astronomy and Astrophysics, volume 411483-487 (2003/12-1)

Curious Variables Experiment (CURVE). CCD photometry of QW Serpentis in superoutburst and quiescence.

OLECH A., KEDZIERSKI P., ZLOCZEWSKI K., MULARCZYK K. and WISNIEWSKI M.

Abstract (from CDS):

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 Psh=0.07703(4)days. In the quiescence we observed a double humped wave characterized by a period of P=0.07457(2) days. As both periods obey the Stolz-Schoembs relation with a period excess equal to 3.30±0.06%, the latter period is interpreted as the orbital period of the binary system.

Abstract Copyright: ∼

Journal keyword(s): stars: individual: QW Ser - stars: binaries: close - stars: novae, cataclysmic variables

Simbad objects: 2

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