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Article: Observations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope

TitleObservations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescope
Authors
Abdo, AAAckermann, MAjello, MAllafort, ABaldini, LBallet, JBarbiellini, GBaring, MGBastieri, DBellazzini, RBerenji, BMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNaumannGodo, MNolan, PLNorris, JPNuss, EOhsugi, TBlandford, RDOkumura, AOrlando, EOrmes, JFPaneque, DParent, DPelassa, VPesceRollins, MPierbattista, MPiron, FPohl, MBloom, EDPorter, TARainò, SRando, RRazzano, MReimer, OReposeur, TRitz, SRomani, RWRoth, MSadrozinski, HFWBonamente, ESaz Parkinson, PMSgrò, CSmith, DASmith, PDSpandre, GSpinelli, PStrickman, MSTajima, HTakahashi, HTakahashi, TBorgland, AWTanaka, TThayer, JGThayer, JBThompson, DJTibaldo, LTibolla, OTorres, DFTosti, GTramacere, ATroja, EBouvier, AUchiyama, YVandenbroucke, JVasileiou, VVianello, GVilchez, NVitale, VWaite, APWang, PWiner, BLWood, KSBrandt, TJYamamoto, HYamazaki, RYang, ZZiegler, MBregeon, JBrigida, MBruel, PBuehler, RBuson, SCaliandro, GACameron, RACaraveo, PACasandjian, JMCecchi, CChaty, SChekhtman, ACheung, CCChiang, JCillis, ANCiprini, SClaus, RCohenTanugi, JConrad, JCorbel, SCutini, SDe Angelis, ADe Palma, FDermer, CDDigel, SWDo Couto E Silva, EDrell, PSDrlicaWagner, ADubois, RDumora, DFavuzzi, CFerrara, ECFortin, PFrailis, MFukazawa, YFukui, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrenier, IAGrondin, MHGuiriec, SHadasch, DHanabata, YHarding, AKHayashida, MHayashi, KHays, EHoran, DJackson, MSJóhannesson, GJohnson, ASKamae, TKatagiri, HKataoka, JKerr, MKnödlseder, JKuss, MLande, JLatronico, LLee, SHLemoineGoumard, MLongo, FLoparco, FLovellette, MNLubrano, PMadejski, GMMakeev, AMazziotta, MNMcenery, JEMichelson, PFMignani, RPMitthumsiri, WMizuno, TMoiseev, AA
KeywordsAcceleration Of Particles
Gamma Rays: General
Gamma Rays: Ism
Ism: Individual Objects (Rx J1713.7-3946)
Ism: Supernova Remnants
Radiation Mechanisms: Non-Thermal
Issue Date2011
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205
Citation
Astrophysical Journal Letters, 2011, v. 734 n. 1 How to Cite?
DOI: http://dx.doi.org/10.1088/0004-637X/734/1/28
AbstractWe present observations of the young supernova remnant (SNR) RXJ1713.7-3946 with the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with the SNR. The source is extended with a best-fit extension of 055 ± 004 matching the size of the non-thermal X-ray and TeV gamma-ray emission from the remnant. The positional coincidence and the matching extended emission allow us to identify the LAT source with SNR RXJ1713.7-3946. The spectrum of the source can be described by a very hard power law with a photon index of Γ = 1.5 0.1 that coincides in normalization with the steeper H.E.S.S.-detected gamma-ray spectrum at higher energies. The broadband gamma-ray emission is consistent with a leptonic origin as the dominant mechanism for the gamma-ray emission. © 2011. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188408
ISSN
2041-8205
2023 Impact Factor: 8.8
2023 SCImago Journal Rankings: 2.766
ISI Accession Number ID
WOS:000291026900028
References
References in Scopus

 

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.authorBaring, MGen_US
dc.contributor.authorBastieri, Den_US
dc.contributor.authorBellazzini, Ren_US
dc.contributor.authorBerenji, Ben_US
dc.contributor.authorMonte, Cen_US
dc.contributor.authorMonzani, MEen_US
dc.contributor.authorMorselli, Aen_US
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dc.contributor.authorNaumannGodo, Men_US
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dc.contributor.authorNuss, Een_US
dc.contributor.authorOhsugi, Ten_US
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dc.contributor.authorOrlando, Een_US
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dc.contributor.authorPelassa, Ven_US
dc.contributor.authorPesceRollins, Men_US
dc.contributor.authorPierbattista, Men_US
dc.contributor.authorPiron, Fen_US
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dc.contributor.authorBloom, EDen_US
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dc.contributor.authorRando, Ren_US
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dc.contributor.authorBouvier, Aen_US
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dc.contributor.authorVianello, Gen_US
dc.contributor.authorVilchez, Nen_US
dc.contributor.authorVitale, Ven_US
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dc.contributor.authorYamamoto, Hen_US
dc.contributor.authorYamazaki, Ren_US
dc.contributor.authorYang, Zen_US
dc.contributor.authorZiegler, Men_US
dc.contributor.authorBregeon, Jen_US
dc.contributor.authorBrigida, Men_US
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dc.contributor.authorChiang, Jen_US
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dc.contributor.authorClaus, Ren_US
dc.contributor.authorCohenTanugi, Jen_US
dc.contributor.authorConrad, Jen_US
dc.contributor.authorCorbel, Sen_US
dc.contributor.authorCutini, Sen_US
dc.contributor.authorDe Angelis, Aen_US
dc.contributor.authorDe Palma, Fen_US
dc.contributor.authorDermer, CDen_US
dc.contributor.authorDigel, SWen_US
dc.contributor.authorDo Couto E Silva, Een_US
dc.contributor.authorDrell, PSen_US
dc.contributor.authorDrlicaWagner, Aen_US
dc.contributor.authorDubois, Ren_US
dc.contributor.authorDumora, Den_US
dc.contributor.authorFavuzzi, Cen_US
dc.contributor.authorFerrara, ECen_US
dc.contributor.authorFortin, Pen_US
dc.contributor.authorFrailis, Men_US
dc.contributor.authorFukazawa, Yen_US
dc.contributor.authorFukui, Yen_US
dc.contributor.authorFunk, Sen_US
dc.contributor.authorFusco, Pen_US
dc.contributor.authorGargano, Fen_US
dc.contributor.authorGasparrini, Den_US
dc.contributor.authorGehrels, Nen_US
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dc.contributor.authorGiroletti, Men_US
dc.contributor.authorGlanzman, Ten_US
dc.contributor.authorGodfrey, Gen_US
dc.contributor.authorGrenier, IAen_US
dc.contributor.authorGrondin, MHen_US
dc.contributor.authorGuiriec, Sen_US
dc.contributor.authorHadasch, Den_US
dc.contributor.authorHanabata, Yen_US
dc.contributor.authorHarding, AKen_US
dc.contributor.authorHayashida, Men_US
dc.contributor.authorHayashi, Ken_US
dc.contributor.authorHays, Een_US
dc.contributor.authorHoran, Den_US
dc.contributor.authorJackson, MSen_US
dc.contributor.authorJóhannesson, Gen_US
dc.contributor.authorJohnson, ASen_US
dc.contributor.authorKamae, Ten_US
dc.contributor.authorKatagiri, Hen_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorKerr, Men_US
dc.contributor.authorKnödlseder, Jen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLande, Jen_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLee, SHen_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLovellette, MNen_US
dc.contributor.authorLubrano, Pen_US
dc.contributor.authorMadejski, GMen_US
dc.contributor.authorMakeev, Aen_US
dc.contributor.authorMazziotta, MNen_US
dc.contributor.authorMcenery, JEen_US
dc.contributor.authorMichelson, PFen_US
dc.contributor.authorMignani, RPen_US
dc.contributor.authorMitthumsiri, Wen_US
dc.contributor.authorMizuno, Ten_US
dc.contributor.authorMoiseev, AAen_US
dc.date.accessioned2013-09-03T04:05:32Z-
dc.date.available2013-09-03T04:05:32Z-
dc.date.issued2011en_US
dc.identifier.citationAstrophysical Journal Letters, 2011, v. 734 n. 1en_US
dc.identifier.issn2041-8205en_US
dc.identifier.urihttp://hdl.handle.net/10722/188408-
dc.description.abstractWe present observations of the young supernova remnant (SNR) RXJ1713.7-3946 with the Fermi Large Area Telescope (LAT). We clearly detect a source positionally coincident with the SNR. The source is extended with a best-fit extension of 055 ± 004 matching the size of the non-thermal X-ray and TeV gamma-ray emission from the remnant. The positional coincidence and the matching extended emission allow us to identify the LAT source with SNR RXJ1713.7-3946. The spectrum of the source can be described by a very hard power law with a photon index of Γ = 1.5 0.1 that coincides in normalization with the steeper H.E.S.S.-detected gamma-ray spectrum at higher energies. The broadband gamma-ray emission is consistent with a leptonic origin as the dominant mechanism for the gamma-ray emission. © 2011. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/2041-8205en_US
dc.relation.ispartofAstrophysical Journal Lettersen_US
dc.subjectAcceleration Of Particlesen_US
dc.subjectGamma Rays: Generalen_US
dc.subjectGamma Rays: Ismen_US
dc.subjectIsm: Individual Objects (Rx J1713.7-3946)en_US
dc.subjectIsm: Supernova Remnantsen_US
dc.subjectRadiation Mechanisms: Non-Thermalen_US
dc.titleObservations of the young supernova remnant RX J1713.7-3946 with the Fermi Large Area Telescopeen_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.doi10.1088/0004-637X/734/1/28en_US
dc.identifier.scopuseid_2-s2.0-79958288779en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-79958288779&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume734en_US
dc.identifier.issue1en_US
dc.identifier.isiWOS:000291026900028-
dc.publisher.placeUnited Kingdomen_US
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dc.identifier.scopusauthoridMadejski, GM=7202709535en_US
dc.identifier.scopusauthoridMakeev, A=35274970000en_US
dc.identifier.scopusauthoridMazziotta, MN=35399453800en_US
dc.identifier.scopusauthoridMcEnery, JE=35229539600en_US
dc.identifier.scopusauthoridMichelson, PF=26655530300en_US
dc.identifier.scopusauthoridMignani, RP=16406250300en_US
dc.identifier.scopusauthoridMitthumsiri, W=25724434100en_US
dc.identifier.scopusauthoridMizuno, T=7410011980en_US
dc.identifier.scopusauthoridMoiseev, AA=35353364200en_US
dc.identifier.issnl2041-8205-

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