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Article: The fermi gamma-ray space telescope discovers the pulsar in the young galactic supernova remnant CTA 1

TitleThe fermi gamma-ray space telescope discovers the pulsar in the young galactic supernova remnant CTA 1
Authors
Abdo, AAAckermann, MAtwood, WBBaldini, LBallet, JBarbiellini, GBaring, MGBastieri, DBaughman, BMBechtol, KBellazzini, RMazziotta, MNMcenery, JEMcglynn, SMeurer, CMichelson, PFMineo, TMitthumsiri, WMizuno, TMoiseev, AAMonte, CBerenji, BMonzani, MEMorselli, AMoskalenko, IVMurgia, SNakamori, TNolan, PLNuss, EOhno, MOhsugi, TOkumura, ABlandford, RDOmodei, NOrlando, EOrmes, JFOzaki, MPaneque, DPanetta, JHParent, DPelassa, VPepe, MPesceRollins, MBloom, EDPiano, GPieri, LPiron, FPorter, TARainò, SRando, RRay, PSRazzano, MReimer, AReimer, OBogaert, GReposeur, TRitz, SRochester, LSRodriguez, AYRomani, RWRoth, MRyde, FSadrozinski, HFWSanchez, DSander, ABonamente, ESaz Parkinson, PMSchalk, TLSellerholm, ASgrò, CSiskind, EJSmith, DASmith, PDSpandre, GSpinelli, PStarck, JLBorgland, AWStrickman, MSSuson, DJTajima, HTakahashi, HTakahashi, TTanaka, TThayer, JBThayer, JGThompson, DJThorsett, SEBregeon, JTibaldo, LTorres, DFTosti, GTramacere, AUsher, TLVan Etten, AVilchez, NVitale, VWang, PWatters, KBrez, AWiner, BLWood, KSYasuda, HYlinen, TZiegler, MBrigida, MBruel, PBurnett, THCaliandro, GACameron, RACaraveo, PACarlson, PCasandjian, JMCecchi, CCharles, EChekhtman, ACheung, CCChiang, JCiprini, SClaus, RCohenTanugi, JCominsky, LRConrad, JCutini, SDavis, DSDermer, CDDe Angelis, ADe Palma, FDigel, SWDormody, MDo Couto E Silva, EDrell, PSDubois, RDumora, DEdmonds, YFarnier, CFocke, WBFukazawa, YFunk, SFusco, PGargano, FGasparrini, DGehrels, NGermani, SGiebels, BGiglietto, NGiordano, FGlanzman, TGodfrey, GGrenier, IAGrondin, MHGrove, JEGuillemot, LGuiriec, SHarding, AKHartman, RCHays, EHughes, REJóhannesson, GJohnson, ASJohnson, RPJohnson, TJJohnson, WNKamae, TKanai, YKanbach, GKatagiri, HKawai, NKerr, MKishishita, TKiziltan, BKnödlseder, JKocian, MLKomin, NKuehn, FKuss, MLatronico, LLemoineGoumard, MLongo, FLonjou, VLoparco, FLott, BLovellette, MNLubrano, PMakeev, AMarelli, M
Issue Date2008
PublisherAmerican Association for the Advancement of Science. The Journal's web site is located at http://sciencemag.org
Citation
Science, 2008, v. 322 n. 5905, p. 1218-1221 How to Cite?
DOI: http://dx.doi.org/10.1126/science.1165572
AbstractEnergetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma-ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 × 10?13 seconds per second. Its characteristic age of 104 years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma-ray sources associated with star-forming regions and SNRs are such young pulsars.
Persistent Identifierhttp://hdl.handle.net/10722/188359
ISSN
0036-8075
2023 Impact Factor: 44.7
2023 SCImago Journal Rankings: 11.902
ISI Accession Number ID
WOS:000261033400033
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorAbdo, AAen_US
dc.contributor.authorAckermann, Men_US
dc.contributor.authorAtwood, WBen_US
dc.contributor.authorBaldini, Len_US
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dc.contributor.authorKomin, Nen_US
dc.contributor.authorKuehn, Fen_US
dc.contributor.authorKuss, Men_US
dc.contributor.authorLatronico, Len_US
dc.contributor.authorLemoineGoumard, Men_US
dc.contributor.authorLongo, Fen_US
dc.contributor.authorLonjou, Ven_US
dc.contributor.authorLoparco, Fen_US
dc.contributor.authorLott, Ben_US
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dc.date.accessioned2013-09-03T04:03:40Z-
dc.date.available2013-09-03T04:03:40Z-
dc.date.issued2008en_US
dc.identifier.citationScience, 2008, v. 322 n. 5905, p. 1218-1221en_US
dc.identifier.issn0036-8075en_US
dc.identifier.urihttp://hdl.handle.net/10722/188359-
dc.description.abstractEnergetic young pulsars and expanding blast waves [supernova remnants (SNRs)] are the most visible remains after massive stars, ending their lives, explode in core-collapse supernovae. The Fermi Gamma-Ray Space Telescope has unveiled a radio quiet pulsar located near the center of the compact synchrotron nebula inside the supernova remnant CTA 1. The pulsar, discovered through its gamma-ray pulsations, has a period of 316.86 milliseconds and a period derivative of 3.614 × 10?13 seconds per second. Its characteristic age of 104 years is comparable to that estimated for the SNR. We speculate that most unidentified Galactic gamma-ray sources associated with star-forming regions and SNRs are such young pulsars.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.titleThe fermi gamma-ray space telescope discovers the pulsar in the young galactic supernova remnant CTA 1en_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.1165572en_US
dc.identifier.scopuseid_2-s2.0-57149104772en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-57149104772&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume322en_US
dc.identifier.issue5905en_US
dc.identifier.spage1218en_US
dc.identifier.epage1221en_US
dc.identifier.isiWOS:000261033400033-
dc.publisher.placeUnited Statesen_US
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dc.identifier.issnl0036-8075-

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