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Conference Paper: Chandra observations of the high-magnetic-field radio pulsar J1718-3718

TitleChandra observations of the high-magnetic-field radio pulsar J1718-3718
Authors
Zhu, WKaspi, VMMclaughlin, MAPavlov, GGNg, CYManchester, RNGaensler, BMWoods, PM
KeywordsPulsars: Individual (Psr J1718-3718)
Stars: Neutron
X-Rays: Stars
Issue Date2011
PublisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/
Citation
AIP Conference Proceedings, 2011, v. 1379 n. 1, p. 70-73 How to Cite?
DOI: http://dx.doi.org/10.1063/1.3629487
AbstractWe report on four Chandra observations of the high-magnetic-field pulsar J1718-3718 taken in 2009 as well as a re-analysis of 2002 Chandra observations. We detect clear pulsations at the pulsar's period in the 2009 data. We found that the pulsar's X-ray radiation is mostly thermal emission with a blackbody temperature of 186 -18 +19eV. The pulsar's properties are compared to that of some high-magnetic-field pulsars and normal pulsars. Implications of our findings are discussed. © 2011 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/180718
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152
ISI Accession Number ID
WOS:000302936600012
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorZhu, Wen_US
dc.contributor.authorKaspi, VMen_US
dc.contributor.authorMclaughlin, MAen_US
dc.contributor.authorPavlov, GGen_US
dc.contributor.authorNg, CYen_US
dc.contributor.authorManchester, RNen_US
dc.contributor.authorGaensler, BMen_US
dc.contributor.authorWoods, PMen_US
dc.date.accessioned2013-01-28T01:41:46Z-
dc.date.available2013-01-28T01:41:46Z-
dc.date.issued2011en_US
dc.identifier.citationAIP Conference Proceedings, 2011, v. 1379 n. 1, p. 70-73-
dc.identifier.issn0094-243Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/180718-
dc.description.abstractWe report on four Chandra observations of the high-magnetic-field pulsar J1718-3718 taken in 2009 as well as a re-analysis of 2002 Chandra observations. We detect clear pulsations at the pulsar's period in the 2009 data. We found that the pulsar's X-ray radiation is mostly thermal emission with a blackbody temperature of 186 -18 +19eV. The pulsar's properties are compared to that of some high-magnetic-field pulsars and normal pulsars. Implications of our findings are discussed. © 2011 American Institute of Physics.en_US
dc.languageengen_US
dc.publisherAmerican Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/-
dc.relation.ispartofAIP Conference Proceedingsen_US
dc.subjectPulsars: Individual (Psr J1718-3718)en_US
dc.subjectStars: Neutronen_US
dc.subjectX-Rays: Starsen_US
dc.titleChandra observations of the high-magnetic-field radio pulsar J1718-3718en_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.doi10.1063/1.3629487en_US
dc.identifier.scopuseid_2-s2.0-80053363179en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-80053363179&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume1379en_US
dc.identifier.issue1-
dc.identifier.spage70en_US
dc.identifier.epage73en_US
dc.identifier.isiWOS:000302936600012-
dc.publisher.placeUnited Statesen_US
dc.identifier.scopusauthoridZhu, W=55483175400en_US
dc.identifier.scopusauthoridKaspi, VM=7006755510en_US
dc.identifier.scopusauthoridMcLaughlin, MA=7202285147en_US
dc.identifier.scopusauthoridPavlov, GG=16492673600en_US
dc.identifier.scopusauthoridNg, CY=24830903500en_US
dc.identifier.scopusauthoridManchester, RN=7004270810en_US
dc.identifier.scopusauthoridGaensler, BM=34769921200en_US
dc.identifier.scopusauthoridWoods, PM=35560112800en_US
dc.identifier.issnl0094-243X-

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