Diffuse galactic Gamma-rays from star clusters

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7716

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DC Field	Value	Language
dc.contributor.author	Nath, Biman B.	-
dc.contributor.author	Eichler, David	-
dc.date.accessioned	2021-03-04T05:28:10Z	-
dc.date.available	2021-03-04T05:28:10Z	-
dc.date.issued	2020-11	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society , 2020, Vol. 499, Iss. 1, p.L1 - L5	en_US
dc.identifier.issn	0035-8711	-
dc.identifier.issn	1365-2966 - (online)	-
dc.identifier.uri	http://hdl.handle.net/2289/7716	-
dc.description	Open Access	en_US
dc.description.abstract	We 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.language.iso	en	en_US
dc.publisher	Oxford University Press for the RAS	en_US
dc.relation.uri	https://academic.oup.com/mnrasl/article/499/1/L1/5898124	en_US
dc.relation.uri	https://arxiv.org/abs/2008.11220	en_US
dc.rights	2020 The authors & the Royal Astronomical Society.	en_US
dc.subject	ISM	en_US
dc.subject	bubbles – ISM	en_US
dc.subject	Cosmic rays – gamma-rays	en_US
dc.subject	diffuse background	en_US
dc.title	Diffuse galactic Gamma-rays from star clusters	en_US
dc.type	Article	en_US
Appears in Collections:	Research Papers (A&A)

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