pγ interactions in Galactic jets as a plausible origin of the positron excess

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DC Field	Value	Language
dc.contributor.author	Gupta, Nayantara	-
dc.contributor.author	Torres, Diego F.	-
dc.date.accessioned	2014-09-11T12:25:37Z	-
dc.date.available	2014-09-11T12:25:37Z	-
dc.date.issued	2014-07-04	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, 2014, Vol. 441, p3122-3126	en
dc.identifier.issn	0035-8711	-
dc.identifier.issn	1365-2966 - (online)	-
dc.identifier.uri	http://hdl.handle.net/2289/5968	-
dc.description	Open Access.	en
dc.description.abstract	The positron flux measured near Earth shows a rise with energy beyond 30 GeV. We show that this rise might be compatible with the production of positrons in pγ interactions in the jets of microquasars.	en
dc.language.iso	en	en
dc.publisher	Oxford University Press	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2014MNRAS.441.3122G	en
dc.relation.uri	http://arxiv.org/abs/1404.4188	en
dc.relation.uri	http://dx.doi.org/10.1093/mnras/stu770	en
dc.rights	2014 The authors & the Royal Astronomical Society	en
dc.subject	Cosmic rays	en
dc.subject	Galaxy centre	en
dc.title	pγ interactions in Galactic jets as a plausible origin of the positron excess	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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