Izzo, L.L.IzzoDELLA VALLE, MassimoMassimoDELLA VALLEEderoclite, A.A.EderocliteHenze, M.M.Henze2020-04-242020-04-242015978-80-01-05688-2978-80-905129-3-12336-5382http://hdl.handle.net/20.500.12386/24232We 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⊙STAMPAenConference paper10.14311/APP.2015.02.0264https://ojs.cvut.cz/ojs/index.php/APP/article/view/29182015AcPPP...2..264IFIS/05 - ASTRONOMIA E ASTROFISICA