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 |
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