The Nova V5584 Sgr: A Short Review
dc.contributor.author | Poggiani, R. | |
dc.date.accessioned | 2023-01-18T14:26:44Z | |
dc.date.available | 2023-01-18T14:26:44Z | |
dc.date.issued | 2015 | |
dc.identifier.citation | Acta Polytechnica. 2015, vol. 2, no. 1, p. 234-237. | |
dc.identifier.issn | 1210-2709 (print) | |
dc.identifier.issn | 1805-2363 (online) | |
dc.identifier.uri | http://hdl.handle.net/10467/105790 | |
dc.description.abstract | The nova V5584 Sgr was discovered during 2009 October. It has been monitored in different domains of the electromagnetic spectrum: optical, infrared and X-rays. The optical and infrared observations suggest that V5584 Sgr is a Fe II nova that formed dust. No X-ray emission was observed around the time of maximum. | 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/2905 | |
dc.rights | Creative Commons Attribution 4.0 International License | en |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | |
dc.title | The Nova V5584 Sgr: A Short Review | |
dc.type | article | en |
dc.date.updated | 2023-01-18T14:26:44Z | |
dc.identifier.doi | 10.14311/APP.2015.02.0234 | |
dc.rights.access | openAccess | |
dc.type.status | Peer-reviewed | |
dc.type.version | publishedVersion |
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