학술논문
On the 2011 Outburst of the Recurrent Nova T Pyxidis
Document Type
article
Author
Source
Acta Polytechnica CTU Proceedings, Vol 2, Iss 1, Pp 264-268 (2015)
Subject
Language
English
ISSN
2336-5382
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.