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Paper detail

V2491 Cyg - a possible recurrent nova ?

Nova V2491 Cyg was discovered on April 10.72 UT 2008 (Nakano, 2008). Here we present spectrophotometric premises that V2491 Cyg can be a good candidate for recurrent nova (RNe). Its properties are compared to five well known RNe with red dwarf secondaries (U Sco, V394 Cra, T Pyx, CI Aql, IM Nor) and recently confirmed as recurrent nova V2487 Oph (Pagnotta et al.,2008). Photometric $U, B, V, R_C, I_C$ and moderate resolution (R$\sim 1500$) spectral observations of V2491 Cyg were carried out in the Torun Observatory (Poland) between April 14 and May 20 2008.

preprint2010arXivOpen access
E. RaganM. MikolajewskiT. TomovE. SwierczynskiT. BrozekC. GalanP. RozanskiM. WiecekP. Wychudzki
astro-ph.SR
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E. RaganM. MikolajewskiT. TomovE. SwierczynskiT. BrozekC. GalanP. RozanskiM. WiecekP. Wychudzki

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