Are Supernovae Responsible for the Gamma Ray Spectrum from the Galactic Center?

dc.contributor.author	Stanev, Todor
dc.date.accessioned	2023-01-18T14:11:42Z
dc.date.available	2023-01-18T14:11:42Z
dc.date.issued	2014
dc.identifier.citation	Acta Polytechnica. 2014, vol. 1, no. 1, p. 189-193.
dc.identifier.issn	1210-2709 (print)
dc.identifier.issn	1805-2363 (online)
dc.identifier.uri	http://hdl.handle.net/10467/105713
dc.description.abstract	We discuss the supernova remnants distribution as a function of the galactic longitude and compare their positions to that of the detected TeV gamma ray sources. A large fraction of these sources either coincide or a close by known supernova remnants. If we look within 10o of the Galactic center most identied sources are combinations of supernova remnants with giant molecular clouds. The diffuse gamma ray flux from the direction of the Galactic center is much smaller.	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/2383
dc.rights	Creative Commons Attribution 4.0 International License	en
dc.rights.uri	http://creativecommons.org/licenses/by/4.0/
dc.title	Are Supernovae Responsible for the Gamma Ray Spectrum from the Galactic Center?
dc.type	article	en
dc.date.updated	2023-01-18T14:11:42Z
dc.identifier.doi	10.14311/APP.2014.01.0189
dc.rights.access	openAccess
dc.type.status	Peer-reviewed
dc.type.version	publishedVersion

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