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Article: Gamma-ray pulsars in the Fermi LAT era

TitleGamma-ray pulsars in the Fermi LAT era
Authors
Issue Date2011
Citation
Nuovo Cimento Della Societa Italiana Di Fisica C, 2011, v. 34 n. 3, p. 173-178 How to Cite?
AbstractObservations over the past two years with the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope have led to a tenfold increase in the number of known γ-ray pulsars. Roughly one third of this population consists of young radio-loud pulsars, one third are radio-quiet pulsars discovered in blind searches of LAT data, and one third are γ-ray millisecond pulsars (MSPs). In this paper I discuss what we have learned about these three populations, as well as prospects for further discoveries. © Società Italiana di Fisica.
Persistent Identifierhttp://hdl.handle.net/10722/188429
ISSN
2008 Impact Factor: 0.277
2015 SCImago Journal Rankings: 0.204
References

 

DC FieldValueLanguage
dc.contributor.authorSaz Parkinson, PMen_US
dc.date.accessioned2013-09-03T04:05:53Z-
dc.date.available2013-09-03T04:05:53Z-
dc.date.issued2011en_US
dc.identifier.citationNuovo Cimento Della Societa Italiana Di Fisica C, 2011, v. 34 n. 3, p. 173-178en_US
dc.identifier.issn1124-1896en_US
dc.identifier.urihttp://hdl.handle.net/10722/188429-
dc.description.abstractObservations over the past two years with the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope have led to a tenfold increase in the number of known γ-ray pulsars. Roughly one third of this population consists of young radio-loud pulsars, one third are radio-quiet pulsars discovered in blind searches of LAT data, and one third are γ-ray millisecond pulsars (MSPs). In this paper I discuss what we have learned about these three populations, as well as prospects for further discoveries. © Società Italiana di Fisica.en_US
dc.languageengen_US
dc.relation.ispartofNuovo Cimento della Societa Italiana di Fisica Cen_US
dc.titleGamma-ray pulsars in the Fermi LAT eraen_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.doi10.1393/ncc/i2011-10888-7en_US
dc.identifier.scopuseid_2-s2.0-84870395434en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-84870395434&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume34en_US
dc.identifier.issue3en_US
dc.identifier.spage173en_US
dc.identifier.epage178en_US
dc.identifier.scopusauthoridSaz Parkinson, PM=8948464400en_US

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