On the 2011 Outburst of the Recurrent Nova T Pyxidis

Authors

  • L. Izzo Dip. di Fisica, Sapienza University of Rome, P.le A. Moro 2, Rome; ICRANet, P.le della Repubblica 10, Pescara, Italy
  • M. della Valle INAF - Osservatorio di Capodimonte, Salita Moiariello 16, 80131 Napoli, Italy
  • A. Ederoclite Centro de Estudios de Fisica del Cosmos de Aragon, Plaza San Juan 1, Planta 2, Teruel, E44001, Spain
  • M. Henze European Space Astronomy Centre, P.O. Box 78, 28692 Villanueva de la Canada, Madrid, Spain

DOI:

https://doi.org/10.14311/APP.2015.02.0264

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.

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Published

2015-02-23

How to Cite

Izzo, L., della Valle, M., Ederoclite, A., & Henze, M. (2015). On the 2011 Outburst of the Recurrent Nova T Pyxidis. Acta Polytechnica CTU Proceedings, 2(1), 264–268. https://doi.org/10.14311/APP.2015.02.0264

Issue

Vol. 2 No. 1 (2015): THE GOLDEN AGE OF CATACLYSMIC VARIABLES AND RELATED OBJECTS - II

Section

Articles