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Article: Modulated high-energy gamma-ray emission from the microquasar Cygnus X-3

TitleModulated high-energy gamma-ray emission from the microquasar Cygnus X-3
Authors
Abdo, AAAckermann, MAjello, MAxelsson, MBaldini, LBallet, JBarbiellini, GBastieri, DBaughman, BMBechtol, KBellazzini, RMazziotta, MNMccoll, NMcenery, JEMeurer, CMichelson, PFMigliari, SMitthumsiri, WMizuno, TMonte, CMonzani, MEBerenji, BMorselli, AMoskalenko, IVMurgia, SNolan, PLNorris, JPNuss, EOhsugi, TOmodei, NOng, RAOrmes, JFBlandford, RDPaneque, DParent, DPelassa, VPepe, MPesceRollins, MPiron, FPooley, GPorter, TAPottschmidt, KRainò, SBloom, EDRando, RRay, PSRazzano, MRea, NReadhead, AReimer, AReimer, ORichards, JLRochester, LSRodriguez, JBonamente, ERodriguez, AYRomani, RWRyde, FSadrozinski, HFWSander, ASaz Parkinson, PMSgrò, CSiskind, EJSmith, DASmith, PDBorgland, AWSpinelli, PStarck, JLStevenson, MStrickman, MSSuson, DJTakahashi, HTanaka, TThayer, JBThompson, DJTibaldo, LBrez, ATomsick, JATorres, DFTosti, GTramacere, AUchiyama, YUsher, TLVasileiou, VVilchez, NVitale, VWaite, APBrigida, MWang, PWilms, JWiner, BLWood, KSYlinen, TZiegler, MBruel, PBurnett, THBuson, SCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CÇelik, ÖChaty, SCheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JCominsky, LRConrad, JCorbel, SCorbet, RDermer, CDDe Palma, FDigel, SWDo Couto E Silva, EDrell, PSDubois, RDubus, GDumora, DFarnier, CFavuzzi, CFegan, SJFocke, WBFortin, PFrailis, MFusco, PGargano, FGehrels, NGermani, SGiavitto, GGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHanabata, YHarding, AKHayashida, MHays, EHill, ABHjalmarsdotter, LHoran, DHughes, REJackson, MSJóhannesson, GJohnson, ASJohnson, TJJohnson, WNKamae, TKatagiri, HKawai, NKerr, MKnödlseder, JKocian, MLKoerding, EKuss, MLande, JLatronico, LLemoineGoumard, MLongo, FLoparco, FLott, BLovellette, MNLubrano, PMadejski, GMMakeev, AMarchand, LMarelli, MMaxMoerbeck, W
Issue Date2009
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2009, v. 326 n. 5959, p. 1512-1516 How to Cite?
DOI: http://dx.doi.org/10.1126/science.1182174
AbstractMicroquasars are accreting black holes or neutron stars in binary systems with associated relativistic jets. Despite their frequent outburst activity, they have never been unambiguously detected emitting high-energy gamma rays. The Fermi Large Area Telescope (LAT) has detected a variable high-energy source coinciding with the position of the x-ray binary and microquasar Cygnus X-3. Its identification with Cygnus X-3 is secured by the detection of its orbital period in gamma rays, as well as the correlation of the LAT flux with radio emission from the relativistic jets of Cygnus X-3. The gamma-ray emission probably originates from within the binary system, opening new areas in which to study the formation of relativistic jets.
Persistent Identifierhttp://hdl.handle.net/10722/188370
ISSN
0036-8075
2023 Impact Factor: 44.7
2023 SCImago Journal Rankings: 11.902
ISI Accession Number ID
WOS:000272623600051
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAjello, Men_US
dc.contributor.authorAxelsson, Men_US
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dc.contributor.authorBallet, Jen_US
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dc.contributor.authorLoparco, Fen_US
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dc.date.accessioned2013-09-03T04:04:07Z-
dc.date.available2013-09-03T04:04:07Z-
dc.date.issued2009en_US
dc.identifier.citationScience, 2009, v. 326 n. 5959, p. 1512-1516en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188370-
dc.description.abstractMicroquasars are accreting black holes or neutron stars in binary systems with associated relativistic jets. Despite their frequent outburst activity, they have never been unambiguously detected emitting high-energy gamma rays. The Fermi Large Area Telescope (LAT) has detected a variable high-energy source coinciding with the position of the x-ray binary and microquasar Cygnus X-3. Its identification with Cygnus X-3 is secured by the detection of its orbital period in gamma rays, as well as the correlation of the LAT flux with radio emission from the relativistic jets of Cygnus X-3. The gamma-ray emission probably originates from within the binary system, opening new areas in which to study the formation of relativistic jets.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.titleModulated high-energy gamma-ray emission from the microquasar Cygnus X-3en_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.1182174en_US
dc.identifier.scopuseid_2-s2.0-72149106222en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-72149106222&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume326en_US
dc.identifier.issue5959en_US
dc.identifier.spage1512en_US
dc.identifier.epage1516en_US
dc.identifier.isiWOS:000272623600051-
dc.publisher.placeUnited Statesen_US
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dc.identifier.scopusauthoridKerr, M=6701783498en_US
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dc.identifier.scopusauthoridMaxMoerbeck, W=7404848681en_US
dc.identifier.issnl0036-8075-

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