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dc.contributor.authorBagoly , Z.
dc.contributor.authorVeres , P.
dc.contributor.authorHorváth , I.
dc.contributor.authorMészáros , A.
dc.contributor.authorBalázs , L. G.
dc.date.accessioned2017-02-03T10:09:55Z
dc.date.available2017-02-03T10:09:55Z
dc.date.issued2012
dc.identifier.citationActa Polytechnica. 2012, vol. 52, no. 1.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/66902
dc.description.abstractGamma-ray bursts are usually classified into either short-duration or long-duration bursts. Going beyond the short-long classification scheme, it has been shown on statistical grounds that a third, intermediate population is needed in this classification scheme. We are looking for physical properties which discriminate the intermediate duration bursts from the other two classes. As the intermediate group is the softest, we argue that we have related them with X-ray flashes among the GRBs. We give a new, probabilistic definition for this class of events.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/ap/article/view/1496
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectgamma raysen
dc.subjectburstsen
dc.subjectobservationsen
dc.titleOn the Relation Between GRB Classes and Xray Flashes
dc.typearticleen
dc.date.updated2017-02-03T10:09:56Z
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Except where otherwise noted, this item's license is described as Creative Commons Attribution 4.0 International License