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[vsnet-alert 4126] Superhump period of RX J0459.7+1926

Superhump period of RX J0459.7+1926

Dear Colleagues,

    The analysis of the time-series CCD photometry provided by Gianluca Masi
and Alessia Cassetti has yielded the superhump period of 0.0682 d.  This
period makes RX J0459.7+1926 one of SU UMa-type dwarf novae with relatively
short orbital periods.  Further observations are strongly encouraged.
The Kyoto team will be observing, weather permitting (getting better).

Regards,
Gianluca Masi, Alessia Cassetti, Patrick Schmeer, Taichi Kato, Makoto Uemura
On behalf of the VSNET RX J0459.7+1926 team

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