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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