On the 2011 outburst of the Recurrent Nova T Pyxidis
  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$\odot$. 
L. Izzo, M. Della Valle, A. Ederoclite, M. Henze
astro-ph.SR