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Article: A cocoon of freshly accelerated cosmic rays detected by fermi in the cygnus superbubble

TitleA cocoon of freshly accelerated cosmic rays detected by fermi in the cygnus superbubble
Authors
Issue Date2011
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2011, v. 334 n. 6059, p. 1103-1107 How to Cite?
AbstractThe origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from the shock and their evolution through the turbulent medium surrounding massive stars. Gamma rays can probe their spreading through the ambient gas and radiation fields. The Fermi Large Area Telescope (LAT) has observed the star-forming region of Cygnus X. The 1- to 100-gigaelectronvolt images reveal a 50-parsec-wide cocoon of freshly accelerated cosmic rays that flood the cavities carved by the stellar winds and ionization fronts from young stellar clusters. It provides an example to study the youth of cosmic rays in a superbubble environment before they merge into the older Galactic population.
Persistent Identifierhttp://hdl.handle.net/10722/188414
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
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dc.contributor.authorSaz Parkinson, PMen_US
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dc.date.accessioned2013-09-03T04:05:39Z-
dc.date.available2013-09-03T04:05:39Z-
dc.date.issued2011en_US
dc.identifier.citationScience, 2011, v. 334 n. 6059, p. 1103-1107en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188414-
dc.description.abstractThe origin of Galactic cosmic rays is a century-long puzzle. Indirect evidence points to their acceleration by supernova shockwaves, but we know little of their escape from the shock and their evolution through the turbulent medium surrounding massive stars. Gamma rays can probe their spreading through the ambient gas and radiation fields. The Fermi Large Area Telescope (LAT) has observed the star-forming region of Cygnus X. The 1- to 100-gigaelectronvolt images reveal a 50-parsec-wide cocoon of freshly accelerated cosmic rays that flood the cavities carved by the stellar winds and ionization fronts from young stellar clusters. It provides an example to study the youth of cosmic rays in a superbubble environment before they merge into the older Galactic population.en_US
dc.languageengen_US
dc.publisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.orgen_US
dc.relation.ispartofScienceen_US
dc.titleA cocoon of freshly accelerated cosmic rays detected by fermi in the cygnus superbubbleen_US
dc.typeArticleen_US
dc.identifier.emailSaz Parkinson, PM: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, PM=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1126/science.1210311en_US
dc.identifier.pmid22116880-
dc.identifier.scopuseid_2-s2.0-82255195528en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-82255195528&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume334en_US
dc.identifier.issue6059en_US
dc.identifier.spage1103en_US
dc.identifier.epage1107en_US
dc.identifier.isiWOS:000297313900042-
dc.publisher.placeUnited Statesen_US
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