Cataclysmic Variables and Gamma-Ray Sources

E. Pavlenko; V. Malanushenko; S. Shugarov; D. Chochol

doi:10.1051/eas/1361039

All issues

Volume 61 (2013)

EAS Publications Series, 61 (2013) 255-257

Abstract

Issue		EAS Publications Series Volume 61, 2013 Gamma-ray Bursts: 15 Years of GRB Afterglows – Progenitors, Environments and Host Galaxies from the Nearby to the Early Universe


Page(s)		255 - 257
Section		Chapter V: Afterglow Emission-I Long GRBs (Observations)
DOI		https://doi.org/10.1051/eas/1361039
Published online		22 July 2013

Gamma-ray Bursts: 15 Years of GRB Afterglows
A.J. Castro-Tirado, J.Gorosabel and I.H. Park (eds)
EAS Publications Series, 61 (2013) 255-257

Cataclysmic Variables and Gamma-Ray Sources

E. Pavlenko¹, V. Malanushenko², S. Shugarov³^,4 and D. Chochol⁴

¹ Crimean Astrophysical Observatory, Crimea, Ukraine
² Apache Point Observatory, New Mexico State University, USA
³ Sternberg Astronomical Institute, Lomonosov Moscow University, Russia
⁴ Astronomical Institute of the Slovak Academy of Sciences, Slovakia

Abstract

The cataclysmic variables are associated with high energy events and probably many of them could be potential gamma-ray sources. Up to now Fermi-LAT detected 3 gamma-ray transients, which belong to CVs and related objects: V407 Cyg, N Sco 2012 and N Mon 2012 = V959 Mon. We present the first multicolour observations of the slow classical nova V959 Mon.