The multifrequency behaviour of the recurrent nova RS Ophiuchi
arXiv:1110.6330 · doi:10.1017/S1743921312019382
Abstract
This review concentrates on the multifrequency behaviour of RS Ophiuchi and in particular during its latest outburst. Confirmation of the 1945 outburst, bipolar outflows and its possible fate as a Type Ia Supernova are discussed.
5 pages, 5 figures, in The Golden Age of Cataclysmic Variables and Related Objects, F. Giovannelli & L. Sabau-Graziati (eds.), Mem. SAIt. 83 N.2 (in press)
References in corpus (4)
- Shape: A 3D Modeling Tool for Astrophysics
- An asymmetric shock wave in the 2006 outburst of the recurrent nova RS Ophiuchi
- Exquisite Nova Light Curves from the Solar Mass Ejection Imager (SMEI)
- The Expanding Nebular Remnant of the Recurrent Nova RS Ophiuchi (2006): II. Modeling of Combined Hubble Space Telescope Imaging and Ground-based Spectroscopy