On the 2011 outburst of the Recurrent Nova T Pyxidis
arXiv:1407.7076
Abstract
We discuss the nebular phase emission during the 2011 outburst of the recurrent nova T Pyxidis and present preliminary results on the analysis of the line profiles. We also present some discussions about the binary system configurations and the X-ray emission, showing that the white dwarf mass should be larger than 0.8 M$\odot$.
Proceedings of the conference "The Golden Age of Cataclysmic Variables and Related Objects II", Palermo, 9-14 September 2013. To be published in Acta Polytechnica. 4 pages, 2 figures