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- Publisher Website: 10.1393/ncc/i2011-10888-7
- Scopus: eid_2-s2.0-84870395434
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Article: Gamma-ray pulsars in the Fermi LAT era
Title | Gamma-ray pulsars in the Fermi LAT era |
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Authors | |
Issue Date | 2011 |
Citation | Nuovo Cimento Della Societa Italiana Di Fisica C, 2011, v. 34 n. 3, p. 173-178 How to Cite? |
Abstract | Observations 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 Identifier | http://hdl.handle.net/10722/188429 |
ISSN | |
ISI Accession Number ID | |
References |
DC Field | Value | Language |
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dc.contributor.author | Saz Parkinson, PM | en_US |
dc.date.accessioned | 2013-09-03T04:05:53Z | - |
dc.date.available | 2013-09-03T04:05:53Z | - |
dc.date.issued | 2011 | en_US |
dc.identifier.citation | Nuovo Cimento Della Societa Italiana Di Fisica C, 2011, v. 34 n. 3, p. 173-178 | en_US |
dc.identifier.issn | 1124-1896 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/188429 | - |
dc.description.abstract | Observations 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.language | eng | en_US |
dc.relation.ispartof | Nuovo Cimento della Societa Italiana di Fisica C | en_US |
dc.title | Gamma-ray pulsars in the Fermi LAT era | en_US |
dc.type | Article | en_US |
dc.identifier.email | Saz Parkinson, PM: pablosp@hku.hk | en_US |
dc.identifier.authority | Saz Parkinson, PM=rp01803 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1393/ncc/i2011-10888-7 | en_US |
dc.identifier.scopus | eid_2-s2.0-84870395434 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-84870395434&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 34 | en_US |
dc.identifier.issue | 3 | en_US |
dc.identifier.spage | 173 | en_US |
dc.identifier.epage | 178 | en_US |
dc.identifier.isi | WOS:000421832500026 | - |
dc.identifier.scopusauthorid | Saz Parkinson, PM=8948464400 | en_US |
dc.identifier.issnl | 1124-1896 | - |