Observations of the Deeply Eclipsing Dwarf Nova Gy Cnc

Details Observations of the Deeply Eclipsing Dwarf Nova Gy Cnc Observations of the Deeply Eclipsing Dwarf Nova Gy Cnc

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.296..469k&link_type=abstract

Astrophysics and Space Science, Volume 296, Issue 1-4, pp. 469-472

Astronomy and Astrophysics

Astrophysics

Binary Stars, Cataclysmic Variables, X-Ray Source

Scientific paper

We present photometric measurements of the eclipsing dwarf nova and
X-ray source GY Cnc. The observations were collected during outbursts
and in quiescence. The investigation of plates from the Sonneberg
archive showed that the mean outburst interval is about 210 270 days,
that the outburst is very fast, and lasts for about 5 days.

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