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Conference Paper: Pulsar wind nebulae in EGRET error boxes

TitlePulsar wind nebulae in EGRET error boxes
Authors
Roberts, MSEBrogan, CLGaensler, BMHessels, JWTNg, CYRomani, RW
KeywordsEgret
Gamma-Ray
Gev J1809-2327
Psr J2021+3651
Pwn
Rabbit
Issue Date2005
PublisherSpringer Verlag Dordrecht. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0004-640X
Citation
Astrophysics And Space Science, 2005, v. 297 n. 1-4, p. 93-100 How to Cite?
DOI: http://dx.doi.org/10.1007/s10509-005-7579-9
AbstractA remarkable number of pulsar wind nebulae (PWN) are coincident with EGRET γ-ray sources. X-ray and radio imaging studies of unidentified EGRET sources have resulted in the discovery of at least six new pulsar wind nebulae (PWN). Stationary PWN (SPWN) appear to be associated with steady EGRET sources with hard spectra, typical for γ-ray pulsars. Their toroidal morphologies can help determine the geometry of the pulsar which is useful for constraining models of pulsed γ-ray emission. Rapidly moving PWN (RPWN) with more cometary morphologies seem to be associated with variable EGRET sources in regions where the ambient medium is dense compared to what is typical for the ISM. © Springer Science + Business Media, Inc. 2005.
Persistent Identifierhttp://hdl.handle.net/10722/180715
ISSN
0004-640X
2021 Impact Factor: 1.909
2020 SCImago Journal Rankings: 0.398
ISI Accession Number ID
WOS:000228545100011
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorRoberts, MSEen_US
dc.contributor.authorBrogan, CLen_US
dc.contributor.authorGaensler, BMen_US
dc.contributor.authorHessels, JWTen_US
dc.contributor.authorNg, CYen_US
dc.contributor.authorRomani, RWen_US
dc.date.accessioned2013-01-28T01:41:44Z-
dc.date.available2013-01-28T01:41:44Z-
dc.date.issued2005en_US
dc.identifier.citationAstrophysics And Space Science, 2005, v. 297 n. 1-4, p. 93-100en_US
dc.identifier.issn0004-640Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/180715-
dc.description.abstractA remarkable number of pulsar wind nebulae (PWN) are coincident with EGRET γ-ray sources. X-ray and radio imaging studies of unidentified EGRET sources have resulted in the discovery of at least six new pulsar wind nebulae (PWN). Stationary PWN (SPWN) appear to be associated with steady EGRET sources with hard spectra, typical for γ-ray pulsars. Their toroidal morphologies can help determine the geometry of the pulsar which is useful for constraining models of pulsed γ-ray emission. Rapidly moving PWN (RPWN) with more cometary morphologies seem to be associated with variable EGRET sources in regions where the ambient medium is dense compared to what is typical for the ISM. © Springer Science + Business Media, Inc. 2005.en_US
dc.languageengen_US
dc.publisherSpringer Verlag Dordrecht. The Journal's web site is located at http://springerlink.metapress.com/openurl.asp?genre=journal&issn=0004-640Xen_US
dc.relation.ispartofAstrophysics and Space Scienceen_US
dc.subjectEgreten_US
dc.subjectGamma-Rayen_US
dc.subjectGev J1809-2327en_US
dc.subjectPsr J2021+3651en_US
dc.subjectPwnen_US
dc.subjectRabbiten_US
dc.titlePulsar wind nebulae in EGRET error boxesen_US
dc.typeConference_Paperen_US
dc.identifier.emailNg, CY: stephen_ng@hku.hken_US
dc.identifier.authorityNg, CY=rp01706en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1007/s10509-005-7579-9en_US
dc.identifier.scopuseid_2-s2.0-17744376994en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-17744376994&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume297en_US
dc.identifier.issue1-4en_US
dc.identifier.spage93en_US
dc.identifier.epage100en_US
dc.identifier.isiWOS:000228545100011-
dc.publisher.placeNetherlandsen_US
dc.identifier.scopusauthoridRoberts, MSE=7404028764en_US
dc.identifier.scopusauthoridBrogan, CL=6603681315en_US
dc.identifier.scopusauthoridGaensler, BM=34769921200en_US
dc.identifier.scopusauthoridHessels, JWT=6701717720en_US
dc.identifier.scopusauthoridNg, CY=24830903500en_US
dc.identifier.scopusauthoridRomani, RW=35248859100en_US
dc.identifier.issnl0004-640X-

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