Outburst Properties of V1504 Cyg and V344 Lyr

dc.contributor.author	Cannizzo, J. K.
dc.date.accessioned	2023-01-18T14:26:11Z
dc.date.available	2023-01-18T14:26:11Z
dc.date.issued	2015
dc.identifier.citation	Acta Polytechnica. 2015, vol. 2, no. 1, p. 156-160.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/105774
dc.description.abstract	I begin by reviewing dwarf novae and the disk instability theory, and then present an overview of three ideas for producing superoutbursts in the SU UMa stars − the thermal tidal instability, irradiation-induced secondary mass overflow, and the plain vanilla disk limit cycle instability. I discuss the properties of the outbursts in two SU UMa systems observed by Kepler in the context of the three theories. I conclude with a look beyond the SU UMa systems.	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/2873
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	Outburst Properties of V1504 Cyg and V344 Lyr
dc.type	article	en
dc.date.updated	2023-01-18T14:26:11Z
dc.identifier.doi	10.14311/APP.2015.02.0156
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

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