On the 2011 Outburst of the Recurrent Nova T Pyxidis

Date Issued
2015
Author(s)
Izzo, L.
•
•
Ederoclite, A.
•
Henze, M.
DOI
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⊙
Coverage
The Golden Age of Cataclysmic Variables and Related Objects II
Series
Volume
vol. 2, n. 1
Start page
264
Conferenece
The Golden Age of Cataclysmic Variables and Related Objects II
Conferenece place
Palermo, Italy
Conferenece date
9-14 September 2014
Uri
Url
Issn Identifier
2336-5382
Ads BibCode
2015AcPPP...2..264I
Rights
open.access
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