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Diffuse galactic Gamma-rays from star clusters

dc.contributor.authorNath, Biman B
dc.contributor.authorEichler, David
dc.date.accessioned2021-03-04T05:28:10Z
dc.date.available2021-03-04T05:28:10Z
dc.date.issued2020-11
dc.descriptionOpen Accessen_US
dc.description.abstractWe demonstrate that young star clusters have a γ -ray surface brightness comparable to that of the diffuse Galactic emission (DGE), and estimate that their sky coverage in the direction of the inner Galaxy exceeds unity. We therefore suggest that they comprise a significant fraction of the DGE.en_US
dc.identifier.citationMonthly Notices of the Royal Astronomical Society , 2020, Vol. 499, Iss. 1, p.L1 - L5en_US
dc.identifier.issn0035-8711
dc.identifier.issn1365-2966 - (online)
dc.identifier.urihttp://hdl.handle.net/2289/7716
dc.language.isoenen_US
dc.publisherOxford University Press for the RASen_US
dc.relation.urihttps://academic.oup.com/mnrasl/article/499/1/L1/5898124en_US
dc.relation.urihttps://arxiv.org/abs/2008.11220en_US
dc.rights2020 The authors & the Royal Astronomical Society.en_US
dc.subjectISMen_US
dc.subjectbubbles – ISMen_US
dc.subjectCosmic rays – gamma-raysen_US
dc.subjectdiffuse backgrounden_US
dc.titleDiffuse galactic Gamma-rays from star clustersen_US
dc.typeArticleen_US

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