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Conference Paper: Searching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations

TitleSearching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observations
Authors
KeywordsGamma-Ray Pulsars. Fermi.
Pulsar
Pulsar Wind Nebulae
Issue Date2011
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
Proceedings Of The International Astronomical Union, 2011, v. 7 S279, p. 317-318 How to Cite?
AbstractWe report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminosity vs flux ratio between X-and gamma-rays is unusually large compared to usual radio pulsars. © 2012 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/188514
ISSN
2015 SCImago Journal Rankings: 0.105
References

 

DC FieldValueLanguage
dc.contributor.authorAoki, Yen_US
dc.contributor.authorEnomoto, Ten_US
dc.contributor.authorYatsu, Yen_US
dc.contributor.authorKawai, Nen_US
dc.contributor.authorNakamori, Ten_US
dc.contributor.authorKataoka, Jen_US
dc.contributor.authorSaz Parkinson, Pen_US
dc.date.accessioned2013-09-03T04:09:18Z-
dc.date.available2013-09-03T04:09:18Z-
dc.date.issued2011en_US
dc.identifier.citationProceedings Of The International Astronomical Union, 2011, v. 7 S279, p. 317-318en_US
dc.identifier.issn1743-9213en_US
dc.identifier.urihttp://hdl.handle.net/10722/188514-
dc.description.abstractWe report the Suzaku follow-up observations of the Gamma-ray pulsars, 1FGL J0614,13328, J1044.55737, J1741.82101, and J1813.31246, which were discovered by the Fermi Gamma-ray observatory. Analysing Suzaku/XIS data, we detected X-ray counterparts of these pulsars in the Fermi error circle and interpreted their spectra with absorbed power-law functions. These results indicate that the origin of these X-ray sources is non-thermal emission from the pulsars or from Pulsar Wind Nebulae (PWNe) surrounding them. Moreover we found that J1741.82101 exhibits a peculiar profile: spin-down luminosity vs flux ratio between X-and gamma-rays is unusually large compared to usual radio pulsars. © 2012 International Astronomical Union.en_US
dc.languageengen_US
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAUen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectGamma-Ray Pulsars. Fermi.en_US
dc.subjectPulsaren_US
dc.subjectPulsar Wind Nebulaeen_US
dc.titleSearching for X-ray counterparts of fermi gamma-ray pulsars in suzaku observationsen_US
dc.typeConference_Paperen_US
dc.identifier.emailSaz Parkinson, P: pablosp@hku.hken_US
dc.identifier.authoritySaz Parkinson, P=rp01803en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1017/S1743921312013130en_US
dc.identifier.scopuseid_2-s2.0-84866261868en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84866261868&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume7en_US
dc.identifier.issueS279en_US
dc.identifier.spage317en_US
dc.identifier.epage318en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridAoki, Y=55358273700en_US
dc.identifier.scopusauthoridEnomoto, T=36052706400en_US
dc.identifier.scopusauthoridYatsu, Y=10238844100en_US
dc.identifier.scopusauthoridKawai, N=55191405000en_US
dc.identifier.scopusauthoridNakamori, T=8273010400en_US
dc.identifier.scopusauthoridKataoka, J=25637485000en_US
dc.identifier.scopusauthoridSaz Parkinson, P=8948464400en_US

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