On the 2011 Outburst of the Recurrent Nova T Pyxidis

dc.contributor.author	Izzo, L.
dc.contributor.author	della Valle, M.
dc.contributor.author	Ederoclite, A.
dc.contributor.author	Henze, M.
dc.date.accessioned	2023-01-18T14:27:13Z
dc.date.available	2023-01-18T14:27:13Z
dc.date.issued	2015
dc.identifier.citation	Acta Polytechnica. 2015, vol. 2, no. 1, p. 264-268.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/105797
dc.description.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.	en
dc.format.mimetype	application/pdf
dc.language.iso	eng
dc.publisher	České vysoké učení technické v Praze	cs
dc.publisher	Czech Technical University in Prague	en
dc.relation.ispartofseries	Acta Polytechnica
dc.relation.uri	https://ojs.cvut.cz/ojs/index.php/APP/article/view/2918
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	On the 2011 Outburst of the Recurrent Nova T Pyxidis
dc.type	article	en
dc.date.updated	2023-01-18T14:27:13Z
dc.identifier.doi	10.14311/APP.2015.02.0264
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License