V2491 Cyg - a possible recurrent nova?

Details V2491 Cyg - a possible recurrent nova? V2491 Cyg - a possible recurrent nova?

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1485....1t&link_type=abstract

The Astronomer's Telegram, #1485

Astronomy and Astrophysics

Astronomy

14

Optical, Binaries, Cataclysmic Variables, Novae, Stars

Scientific paper

We report on further optical observations of nova V2491 Cyg obtained in the Piwnice Observatory (Torun, Poland). Spectral observations were secured with the Canadian Copernicus Spectrograph attached to the 60/90 cm Schmidt-Cassegrain telescope. The UBVRI photometry was carried out with the 60 cm Cassegrain telescope. Our brightness estimations obtained on Apr. 14.99 UT were 9.23, 9.53, 9.33, 8.28, 8.01 for UBVRI, respectively; on Apr.

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