Photometric Study of SU UMa-type Dwarf Nova 1RXP J1131.23+4322.5

Details Photometric Study of SU UMa-type Dwarf Nova 1RXP J1131.23+4322.5 Photometric Study of SU UMa-type Dwarf Nova 1RXP J1131.23+4322.5

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..362..207t&link_type=abstract

The Seventh Pacific Rim Conference on Stellar Astrophysics, ASP Conference Series, Vol. 362, Proceedings of the conference held

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

We report our observation and analysis of the three superoutbursts (2003, 2004 and 2005) of the SU UMa-type dwarf nova 1RXP J113123 +4322.5 discovered by ROSAT. Most of the observations were done by our university team. Observations done by others (VSNET collaboration team) are also combined with our data. As a result, we have detected a superhump period of approximately 0.065 day. We also confirmed the system's supercycle to be close to one year.

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