The Orbital Period and Variability of the Dwarf Nova WW Ceti

Details The Orbital Period and Variability of the Dwarf Nova WW Ceti The Orbital Period and Variability of the Dwarf Nova WW Ceti

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....111.2077r&link_type=abstract

Astronomical Journal v.111, p.2077

Astronomy and Astrophysics

Astronomy

18

Stars: Individual: Ww Ceti, Stars: Cataclysmic Variables

Scientific paper

A radial velocity study resolves a long-standing aliasing problem and shows that the orbital period of the dwarf nova WW Ceti is 0.17578±0.00013 d (4.22 h). Its long-term light curves from RoboScope, AAVSO, Harvard archive, and VSS, RASNZ observations are examined. WW Ceti does not have the characteristic standstills of the Z Cam stars, but does wander in quiescence by well over 1 mag.

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