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 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...

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Main Authors: L. Izzo, M. della Valle, A. Ederoclite, M. Henze
Format: Article
Language:English
Published: CTU Central Library 2015-02-01
Series:Acta Polytechnica CTU Proceedings
Online Access:https://ojs.cvut.cz/ojs/index.php/APP/article/view/2918
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author L. Izzo
M. della Valle
A. Ederoclite
M. Henze
author_facet L. Izzo
M. della Valle
A. Ederoclite
M. Henze
author_sort L. Izzo
collection DOAJ
description 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 M<sub>Θ</sub>.
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spelling doaj.art-f8d00fcb7b554a6b8c2ad1e23a732c232022-12-21T23:28:09ZengCTU Central LibraryActa Polytechnica CTU Proceedings2336-53822015-02-012126426810.14311/APP.2015.02.02642678On the 2011 Outburst of the Recurrent Nova T PyxidisL. Izzo0M. della Valle1A. Ederoclite2M. Henze3Dip. di Fisica, Sapienza University of Rome, P.le A. Moro 2, Rome; ICRANet, P.le della Repubblica 10, Pescara, ItalyINAF - Osservatorio di Capodimonte, Salita Moiariello 16, 80131 Napoli, ItalyCentro de Estudios de Fisica del Cosmos de Aragon, Plaza San Juan 1, Planta 2, Teruel, E44001, SpainEuropean Space Astronomy Centre, P.O. Box 78, 28692 Villanueva de la Canada, Madrid, SpainWe 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 M<sub>Θ</sub>.https://ojs.cvut.cz/ojs/index.php/APP/article/view/2918
spellingShingle L. Izzo
M. della Valle
A. Ederoclite
M. Henze
On the 2011 Outburst of the Recurrent Nova T Pyxidis
Acta Polytechnica CTU Proceedings
title On the 2011 Outburst of the Recurrent Nova T Pyxidis
title_full On the 2011 Outburst of the Recurrent Nova T Pyxidis
title_fullStr On the 2011 Outburst of the Recurrent Nova T Pyxidis
title_full_unstemmed On the 2011 Outburst of the Recurrent Nova T Pyxidis
title_short On the 2011 Outburst of the Recurrent Nova T Pyxidis
title_sort on the 2011 outburst of the recurrent nova t pyxidis
url https://ojs.cvut.cz/ojs/index.php/APP/article/view/2918
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AT aederoclite onthe2011outburstoftherecurrentnovatpyxidis
AT mhenze onthe2011outburstoftherecurrentnovatpyxidis