On the 2011 Outburst of the Recurrent Nova T Pyxidis

L. Izzo, M. della Valle, A. Ederoclite, M. Henze

Abstract


We discuss the nebular phase emission during the 2011 outburst of the recurrent nova T Pyxidis and present preliminaryresults 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 MΘ.

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ISSN 2336-5382 (Online)
Published by the Czech Technical University in Prague