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Fermi bubbles: Giant, multibillion-year-old reservoirs of galactic center cosmic rays

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dc.contributor.authorCrocker, Roland
dc.contributor.authorAharonian, Felix
dc.date.accessioned2015-12-13T22:41:29Z
dc.date.issued2011
dc.date.updated2016-02-24T09:33:17Z
dc.description.abstractRecently evidence has emerged for enormous features in the γ-ray sky observed by the Fermi-LAT instrument: bilateral "bubbles" of emission centered on the core of the Galaxy and extending to around ± 10 kpc from the Galactic plane. These structures are
dc.identifier.issn0031-9007
dc.identifier.urihttp://hdl.handle.net/1885/78530
dc.publisherAmerican Physical Society
dc.rightsAuthor/s retain copyrighten_AU
dc.sourcePhysical Review Letters
dc.subjectKeywords: Cosmic ray protons; Galactic Center; Galactic plane; High areal density; Non-thermal microwaves; Order of magnitude; Star formations; Time-scales; Uniform intensity; X-ray emission; X-ray luminosity; Cosmic rays; Population statistics; Luminance
dc.titleFermi bubbles: Giant, multibillion-year-old reservoirs of galactic center cosmic rays
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue10
local.bibliographicCitation.startpage101102
local.contributor.affiliationCrocker, Roland, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationAharonian, Felix, Dublin Institute for Advanced Studies
local.contributor.authoruidCrocker, Roland, u5240609
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.ariespublicationf5625xPUB7158
local.identifier.citationvolume106
local.identifier.doi10.1103/PhysRevLett.106.101102
local.identifier.scopusID2-s2.0-79952597935
local.type.statusPublished Version

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