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...
Main Authors: | , , , |
---|---|
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 |
_version_ | 1828925152752041984 |
---|---|
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>. |
first_indexed | 2024-12-13T23:08:56Z |
format | Article |
id | doaj.art-f8d00fcb7b554a6b8c2ad1e23a732c23 |
institution | Directory Open Access Journal |
issn | 2336-5382 |
language | English |
last_indexed | 2024-12-13T23:08:56Z |
publishDate | 2015-02-01 |
publisher | CTU Central Library |
record_format | Article |
series | Acta Polytechnica CTU Proceedings |
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 |
work_keys_str_mv | AT lizzo onthe2011outburstoftherecurrentnovatpyxidis AT mdellavalle onthe2011outburstoftherecurrentnovatpyxidis AT aederoclite onthe2011outburstoftherecurrentnovatpyxidis AT mhenze onthe2011outburstoftherecurrentnovatpyxidis |