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Article: Constraints on the galactic population of TeV pulsar wind nebulae using fermi large area telescope observations

TitleConstraints on the galactic population of TeV pulsar wind nebulae using fermi large area telescope observations
Authors
Acero, FAckermann, MAjello, MAllafort, ABaldini, LBallet, JBarbiellini, GBastieri, DBechtol, KBellazzini, RBlandford, RDMizuno, TMonte, CMonzani, MEMorselli, AMoskalenko, IVMurgia, SNakamori, TNemmen, RNuss, EOhsugi, TBloom, EDOkumura, AOrienti, MOrlando, EOrmes, JFPaneque, DPanetta, JHPerkins, JSPesceRollins, MPiron, FPivato, GBonamente, EPorter, TARainò, SRando, RRazzano, MReimer, AReimer, OReposeur, TRitz, SRoth, MRousseau, RBottacini, ESaz Parkinson, PMSchulz, ASgrò, CSiskind, EJSmith, DASpandre, GSpinelli, PSuson, DJTakahashi, HTakeuchi, YBrandt, TJThayer, JGThayer, JBThompson, DJTibaldo, LTibolla, OTinivella, MTorres, DFTosti, GTroja, EUchiyama, YBregeon, JVandenbroucke, JVasileiou, VVianello, GVitale, VWerner, MWiner, BLWood, KSYang, ZBrigida, MBruel, PBuehler, RBuson, SCaliandro, GACameron, RACaraveo, PACecchi, CCharles, EChaves, RCGChekhtman, AChiang, JChiaro, GCiprini, SClaus, RCohenTanugi, JConrad, JCutini, SDalton, MD'ammando, FDe Palma, FDermer, CDVenere, LDSilva, EDCEDrell, PSDrlicaWagner, AFalletti, LFavuzzi, CFegan, SJFerrara, ECFocke, WBFranckowiak, AFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGiglietto, NGiordano, FGiroletti, MGlanzman, TGodfrey, GGrégoire, TGrenier, IAGrondin, MHGrove, JEGuiriec, SHadasch, DHanabata, YHarding, AKHayashida, MHayashi, KHays, EHewitt, JHill, ABHoran, DHou, XHughes, REInoue, YJackson, MSJogler, TJóhannesson, GJohnson, ASKamae, TKawano, TKerr, MKnödlseder, JKuss, MLande, JLarsson, SLatronico, LLemoineGoumard, MLongo, FLoparco, FLovellette, MNLubrano, PMarelli, MMassaro, FMayer, MMazziotta, MNMcenery, JEMehault, JMichelson, PFMitthumsiri, W
KeywordsGamma Rays
General
Issue Date2013
PublisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/
Citation
Astrophysical Journal, 2013, v. 773 n. 1 How to Cite?
AbstractPulsar wind nebulae (PWNe) have been established as the most populous class of TeV γ-ray emitters. Since launch, the Fermi Large Area Telescope (LAT) has identified five high-energy (100 MeV < E < 100 GeV) γ-ray sources as PWNe and detected a large number of PWN candidates, all powered by young and energetic pulsars. The wealth of multi-wavelength data available and the new results provided by Fermi-LAT give us an opportunity to find new PWNe and to explore the radiative processes taking place in known ones. The TeV γ-ray unidentified (UNID) sources are the best candidates for finding new PWNe. Using 45 months of Fermi-LAT data for energies above 10 GeV, an analysis was performed near the position of 58 TeV PWNe and UNIDs within 5° of the Galactic plane to establish new constraints on PWN properties and find new clues on the nature of UNIDs. Of the 58 sources, 30 were detected, and this work provides their γ-ray fluxes for energies above 10 GeV. The spectral energy distributions and upper limits, in the multi-wavelength context, also provide new information on the source nature and can help distinguish between emission scenarios, i.e., between classification as a pulsar candidate or as a PWN candidate. Six new GeV PWN candidates are described in detail and compared with existing models. A population study of GeV PWN candidates as a function of the pulsar/PWN system characteristics is presented. © 2013. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/188437
ISSN
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorAcero, Fen_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
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dc.contributor.authorMassaro, Fen_US
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dc.date.accessioned2013-09-03T04:06:02Z-
dc.date.available2013-09-03T04:06:02Z-
dc.date.issued2013en_US
dc.identifier.citationAstrophysical Journal, 2013, v. 773 n. 1en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/188437-
dc.description.abstractPulsar wind nebulae (PWNe) have been established as the most populous class of TeV γ-ray emitters. Since launch, the Fermi Large Area Telescope (LAT) has identified five high-energy (100 MeV < E < 100 GeV) γ-ray sources as PWNe and detected a large number of PWN candidates, all powered by young and energetic pulsars. The wealth of multi-wavelength data available and the new results provided by Fermi-LAT give us an opportunity to find new PWNe and to explore the radiative processes taking place in known ones. The TeV γ-ray unidentified (UNID) sources are the best candidates for finding new PWNe. Using 45 months of Fermi-LAT data for energies above 10 GeV, an analysis was performed near the position of 58 TeV PWNe and UNIDs within 5° of the Galactic plane to establish new constraints on PWN properties and find new clues on the nature of UNIDs. Of the 58 sources, 30 were detected, and this work provides their γ-ray fluxes for energies above 10 GeV. The spectral energy distributions and upper limits, in the multi-wavelength context, also provide new information on the source nature and can help distinguish between emission scenarios, i.e., between classification as a pulsar candidate or as a PWN candidate. Six new GeV PWN candidates are described in detail and compared with existing models. A population study of GeV PWN candidates as a function of the pulsar/PWN system characteristics is presented. © 2013. The American Astronomical Society. All rights reserved.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing, Inc. The Journal's web site is located at http://iopscience.iop.org/0004-637X/en_US
dc.relation.ispartofAstrophysical Journalen_US
dc.subjectGamma Raysen_US
dc.subjectGeneralen_US
dc.titleConstraints on the galactic population of TeV pulsar wind nebulae using fermi large area telescope observationsen_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/773/1/77en_US
dc.identifier.scopuseid_2-s2.0-84881307187en_US
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dc.identifier.volume773en_US
dc.identifier.issue1en_US
dc.identifier.isiWOS:000322531900077-
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dc.identifier.scopusauthoridMitthumsiri, W=25724434100en_US
dc.identifier.issnl0004-637X-

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