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Article: Gamma-ray flares from the Crab Nebula

TitleGamma-ray flares from the Crab Nebula
Authors
Abdo, AAAckermann, MAjello, MAllafort, ABaldini, LBallet, JBarbiellini, GBastieri, DBechtol, KBellazzini, RBerenji, BMcenery, JEMichelson, PFMitthumsiri, WMizuno, TMoiseev, AAMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SBlandford, RDNakamori, TNaumannGodo, MNolan, PLNorris, JPNuss, EOhsugi, TOkumura, AOmodei, NOrmes, JFOzaki, MBloom, EDPaneque, DParent, DPelassa, VPepe, MPesceRollins, MPierbattista, MPiron, FPorter, TARainò, SRando, RBonamente, ERay, PSRazzano, MReimer, AReimer, OReposeur, TRitz, SRomani, RWSadrozinski, HFWSanchez, DSaz Parkinson, PMBorgland, AWScargle, JDSchalk, TLSgrò, CSiskind, EJSmith, PDSpandre, GSpinelli, PStrickman, MSSuson, DJTakahashi, HBouvier, ATakahashi, TTanaka, TThayer, JBThompson, DJTibaldo, LTorres, DFTosti, GTramacere, ATroja, EUchiyama, YBrandt, TJVandenbroucke, JVasileiou, VVianello, GVitale, VWang, PWood, KSYang, ZZiegler, MBregeon, JBrez, ABrigida, MBruel, PBuehler, RBuson, SCaliandro, GACameron, RACannon, ACaraveo, PACasandjian, JMÇelik, ÖCharles, EChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JCostamante, LCutini, SD'ammando, FDermer, CDDe Angelis, ADe Luca, ADe Palma, FDigel, SWDo Couto E Silva, EDrell, PSDrlicaWagner, ADubois, RDumora, DFavuzzi, CFegan, SJFerrara, ECFocke, WBFortin, PFrailis, MFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuiriec, SHadasch, DHanabata, YHarding, AKHayashi, KHayashida, MHays, EHoran, DItoh, RJóhannesson, GJohnson, ASJohnson, TJKhangulyan, DKamae, TKatagiri, HKataoka, JKerr, MKnödlseder, JKuss, MLande, JLatronico, LLee, SHLemoineGoumard, MLongo, FLoparco, FLubrano, PMadejski, GMMakeev, AMarelli, MMazziotta, MN
Issue Date2011
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2011, v. 331 n. 6018, p. 739-742 How to Cite?
AbstractA young and energetic pulsar powers the well-known Crab Nebula. Here, we describe two separate gamma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The first flare occurred in February 2009 and lasted approximately 16 days. The second flare was detected in September 2010 and lasted approximately 4 days. During these outbursts, the gamma-ray flux from the nebula increased by factors of four and six, respectively. The brevity of the flares implies that the gamma rays were emitted via synchrotron radiation from peta-electron-volt (1015 electron volts) electrons in a region smaller than 1.4 × 10-2 parsecs. These are the highest-energy particles that can be associated with a discrete astronomical source, and they pose challenges to particle acceleration theory.
Persistent Identifierhttp://hdl.handle.net/10722/188405
ISSN
2015 Impact Factor: 34.661
2015 SCImago Journal Rankings: 13.217
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAllafort, Aen_US
dc.contributor.authorBaldini, Len_US
dc.contributor.authorBallet, Jen_US
dc.contributor.authorBarbiellini, Gen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBechtol, Ken_US
dc.contributor.authorBellazzini, Ren_US
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dc.contributor.authorMitthumsiri, Wen_US
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dc.contributor.authorJohnson, TJen_US
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dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLubrano, Pen_US
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dc.contributor.authorMarelli, Men_US
dc.contributor.authorMazziotta, MNen_US
dc.date.accessioned2013-09-03T04:05:29Z-
dc.date.available2013-09-03T04:05:29Z-
dc.date.issued2011en_US
dc.identifier.citationScience, 2011, v. 331 n. 6018, p. 739-742en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188405-
dc.description.abstractA young and energetic pulsar powers the well-known Crab Nebula. Here, we describe two separate gamma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The first flare occurred in February 2009 and lasted approximately 16 days. The second flare was detected in September 2010 and lasted approximately 4 days. During these outbursts, the gamma-ray flux from the nebula increased by factors of four and six, respectively. The brevity of the flares implies that the gamma rays were emitted via synchrotron radiation from peta-electron-volt (1015 electron volts) electrons in a region smaller than 1.4 × 10-2 parsecs. These are the highest-energy particles that can be associated with a discrete astronomical source, and they pose challenges to particle acceleration theory.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.titleGamma-ray flares from the Crab Nebulaen_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.1199705en_US
dc.identifier.pmid21212321-
dc.identifier.scopuseid_2-s2.0-79951556096en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-79951556096&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume331en_US
dc.identifier.issue6018en_US
dc.identifier.spage739en_US
dc.identifier.epage742en_US
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dc.identifier.scopusauthoridLongo, F=26425131500en_US
dc.identifier.scopusauthoridLoparco, F=7202709535en_US
dc.identifier.scopusauthoridLubrano, P=35399453800en_US
dc.identifier.scopusauthoridMadejski, GM=35274970000en_US
dc.identifier.scopusauthoridMakeev, A=35229539600en_US
dc.identifier.scopusauthoridMarelli, M=26655530300en_US
dc.identifier.scopusauthoridMazziotta, MN=55725818100en_US

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