Discovery of the First in-the-Gap SUUMa-Type Dwarf Nova, NY Serpentis (=PG 1510+234)

Details Discovery of the First in-the-Gap SUUMa-Type Dwarf Nova, NY Serpentis (=PG 1510+234) Discovery of the First in-the-Gap SUUMa-Type Dwarf Nova, NY Serpentis (=PG 1510+234)

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998pasj...50l...1n&link_type=abstract

Publications of the Astronomical Society of Japan, v.50, p.L1-L4.

Astronomy and Astrophysics

Astronomy

15

Accretion, Accretion Disks, Stars: Dwarf Novae, Stars: Individual (Ny Serpentis), Stars: Variable

Scientific paper

We performed photometric monitoring and time-resolved observations of NY Ser between 1995 July 25 and 1997 March 11. NY Ser shows normal outbursts with a recurrence time of 6--9 days and superoutbursts with a recurrence time of 85--100 days in the range of 14.6--18.0 mag in the V band. The superhump period is 0.106 (+/- 0.001) d, which suggests that the orbital period is located near to the middle of the period gap.

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