Timing observations of rotating radio transients
Identifieur interne : 002965 ( Istex/Curation ); précédent : 002964; suivant : 002966Timing observations of rotating radio transients
Auteurs : M. A. Mclaughlin [États-Unis] ; A. G. Lyne ; E. F. Keane ; M. Kramer [Allemagne] ; J. J. Miller [États-Unis] ; D. R. Lorimer [États-Unis] ; R. N. Manchester [Australie] ; F. Camilo [États-Unis] ; I. H. Stairs [Canada]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2009-12-11.
English descriptors
Abstract
We present radio timing measurements of six rotating radio transient (RRAT) sources discovered in the Parkes Multibeam Pulsar Survey. These provide four new phase‐connected timing solutions and two updated ones, making a total of seven of the original 11 reported RRATs now with high‐precision rotational and astrometric parameters. Three of these seven RRATs have magnetic fields greater than 1013 G, with spin‐down properties similar to those of the magnetars and X‐ray detected isolated neutron stars. Another two of these RRATs have long periods and large characteristic ages, and lie near the ‘death line’ for radio pulsar emission. The remaining two RRATs with timing solutions have properties typical of the bulk of the pulsar population. The new solutions offer insights into what might be responsible for the unusual emission properties. We demonstrate that the RRATs have significantly longer periods and higher magnetic fields than normal radio pulsars, and find no correlation with other spin‐down parameters. These solutions also provide precise positions, which will facilitate follow‐up studies at high energies, crucial for relating these sources with other neutron star populations.
Url:
DOI: 10.1111/j.1365-2966.2009.15584.x
Links toward previous steps (curation, corpus...)
- to stream Istex, to step Corpus: Pour aller vers cette notice dans l'étape Curation :002965
Links to Exploration step
ISTEX:BB8F3730ECC8DBD4A3D2CD1FA4F55F29D184FA5CCuration
No country items
A. G. Lyne<affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation>Le document en format XML
<record><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Timing observations of rotating radio transients</title><author><name sortKey="Mclaughlin, M A" sort="Mclaughlin, M A" uniqKey="Mclaughlin M" first="M. A." last="Mclaughlin">M. A. Mclaughlin</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>National Radio Astronomy Observatory, Green Bank, WV 24944, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>National Radio Astronomy Observatory, Green Bank, WV 24944</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>E-mail: maura.mclaughlin@mail.wvu.edu</mods:affiliation><country wicri:rule="url">États-Unis</country></affiliation></author><author><name sortKey="Lyne, A G" sort="Lyne, A G" uniqKey="Lyne A" first="A. G." last="Lyne">A. G. Lyne</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation></author><author><name sortKey="Keane, E F" sort="Keane, E F" uniqKey="Keane E" first="E. F." last="Keane">E. F. Keane</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation></author><author><name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation><affiliation wicri:level="1"><mods:affiliation>Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany</mods:affiliation><country xml:lang="fr">Allemagne</country><wicri:regionArea>Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn</wicri:regionArea></affiliation></author><author><name sortKey="Miller, J J" sort="Miller, J J" uniqKey="Miller J" first="J. J." last="Miller">J. J. Miller</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation></author><author><name sortKey="Lorimer, D R" sort="Lorimer, D R" uniqKey="Lorimer D" first="D. R." last="Lorimer">D. R. Lorimer</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>National Radio Astronomy Observatory, Green Bank, WV 24944, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>National Radio Astronomy Observatory, Green Bank, WV 24944</wicri:regionArea></affiliation></author><author><name sortKey="Manchester, R N" sort="Manchester, R N" uniqKey="Manchester R" first="R. N." last="Manchester">R. N. Manchester</name><affiliation wicri:level="1"><mods:affiliation>ATNF‐CSIRO, PO Box 76, Epping, NSW 1710, Australia</mods:affiliation><country xml:lang="fr">Australie</country><wicri:regionArea>ATNF‐CSIRO, PO Box 76, Epping, NSW 1710</wicri:regionArea></affiliation></author><author><name sortKey="Camilo, F" sort="Camilo, F" uniqKey="Camilo F" first="F." last="Camilo">F. Camilo</name><affiliation wicri:level="1"><mods:affiliation>Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027</wicri:regionArea></affiliation></author><author><name sortKey="Stairs, I H" sort="Stairs, I H" uniqKey="Stairs I" first="I. H." last="Stairs">I. H. Stairs</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:BB8F3730ECC8DBD4A3D2CD1FA4F55F29D184FA5C</idno><date when="2009" year="2009">2009</date><idno type="doi">10.1111/j.1365-2966.2009.15584.x</idno><idno type="url">https://api-v5.istex.fr/document/BB8F3730ECC8DBD4A3D2CD1FA4F55F29D184FA5C/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">002965</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">002965</idno><idno type="wicri:Area/Istex/Curation">002965</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main" xml:lang="en">Timing observations of rotating radio transients</title><author><name sortKey="Mclaughlin, M A" sort="Mclaughlin, M A" uniqKey="Mclaughlin M" first="M. A." last="Mclaughlin">M. A. Mclaughlin</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>National Radio Astronomy Observatory, Green Bank, WV 24944, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>National Radio Astronomy Observatory, Green Bank, WV 24944</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>E-mail: maura.mclaughlin@mail.wvu.edu</mods:affiliation><country wicri:rule="url">États-Unis</country></affiliation></author><author><name sortKey="Lyne, A G" sort="Lyne, A G" uniqKey="Lyne A" first="A. G." last="Lyne">A. G. Lyne</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation></author><author><name sortKey="Keane, E F" sort="Keane, E F" uniqKey="Keane E" first="E. F." last="Keane">E. F. Keane</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation><wicri:noCountry code="subField">9PL</wicri:noCountry></affiliation></author><author><name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name><affiliation><mods:affiliation>University of Manchester, Jodrell Bank Centre for Astrophysics, Alan Turing Building, Oxford Road, Manchester M13 9PL</mods:affiliation></affiliation><affiliation wicri:level="1"><mods:affiliation>Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany</mods:affiliation><country xml:lang="fr">Allemagne</country><wicri:regionArea>Max Planck Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn</wicri:regionArea></affiliation></author><author><name sortKey="Miller, J J" sort="Miller, J J" uniqKey="Miller J" first="J. J." last="Miller">J. J. Miller</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation></author><author><name sortKey="Lorimer, D R" sort="Lorimer, D R" uniqKey="Lorimer D" first="D. R." last="Lorimer">D. R. Lorimer</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics, West Virginia University, Morgantown, WV 26506, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics, West Virginia University, Morgantown, WV 26506</wicri:regionArea></affiliation><affiliation wicri:level="1"><mods:affiliation>National Radio Astronomy Observatory, Green Bank, WV 24944, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>National Radio Astronomy Observatory, Green Bank, WV 24944</wicri:regionArea></affiliation></author><author><name sortKey="Manchester, R N" sort="Manchester, R N" uniqKey="Manchester R" first="R. N." last="Manchester">R. N. Manchester</name><affiliation wicri:level="1"><mods:affiliation>ATNF‐CSIRO, PO Box 76, Epping, NSW 1710, Australia</mods:affiliation><country xml:lang="fr">Australie</country><wicri:regionArea>ATNF‐CSIRO, PO Box 76, Epping, NSW 1710</wicri:regionArea></affiliation></author><author><name sortKey="Camilo, F" sort="Camilo, F" uniqKey="Camilo F" first="F." last="Camilo">F. Camilo</name><affiliation wicri:level="1"><mods:affiliation>Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027, USA</mods:affiliation><country xml:lang="fr">États-Unis</country><wicri:regionArea>Columbia Astrophysics Laboratory, Columbia University, 550 W. 120th Street, New York, NY 10027</wicri:regionArea></affiliation></author><author><name sortKey="Stairs, I H" sort="Stairs, I H" uniqKey="Stairs I" first="I. H." last="Stairs">I. H. Stairs</name><affiliation wicri:level="1"><mods:affiliation>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1, Canada</mods:affiliation><country xml:lang="fr">Canada</country><wicri:regionArea>Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, BC V6T 1Z1</wicri:regionArea></affiliation></author></analytic><monogr></monogr><series><title level="j">Monthly Notices of the Royal Astronomical Society</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2009-12-11">2009-12-11</date><biblScope unit="volume">400</biblScope><biblScope unit="issue">3</biblScope><biblScope unit="page" from="1431">1431</biblScope><biblScope unit="page" to="1438">1438</biblScope></imprint><idno type="ISSN">0035-8711</idno></series><idno type="istex">BB8F3730ECC8DBD4A3D2CD1FA4F55F29D184FA5C</idno><idno type="DOI">10.1111/j.1365-2966.2009.15584.x</idno><idno type="ArticleID">MNR15584</idno></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Galaxy: stellar content</term><term>pulsars: general</term><term>stars: neutron</term></keywords></textClass><langUsage><language ident="en">en</language></langUsage></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present radio timing measurements of six rotating radio transient (RRAT) sources discovered in the Parkes Multibeam Pulsar Survey. These provide four new phase‐connected timing solutions and two updated ones, making a total of seven of the original 11 reported RRATs now with high‐precision rotational and astrometric parameters. Three of these seven RRATs have magnetic fields greater than 1013 G, with spin‐down properties similar to those of the magnetars and X‐ray detected isolated neutron stars. Another two of these RRATs have long periods and large characteristic ages, and lie near the ‘death line’ for radio pulsar emission. The remaining two RRATs with timing solutions have properties typical of the bulk of the pulsar population. The new solutions offer insights into what might be responsible for the unusual emission properties. We demonstrate that the RRATs have significantly longer periods and higher magnetic fields than normal radio pulsars, and find no correlation with other spin‐down parameters. These solutions also provide precise positions, which will facilitate follow‐up studies at high energies, crucial for relating these sources with other neutron star populations.</div></front></TEI></record>Pour manipuler ce document sous Unix (Dilib)
EXPLOR_STEP=$WICRI_ROOT/Wicri/Canada/explor/ParkinsonCanadaV1/Data/Istex/Curation
HfdSelect -h $EXPLOR_STEP/biblio.hfd -nk 002965 | SxmlIndent | more
Ou
HfdSelect -h $EXPLOR_AREA/Data/Istex/Curation/biblio.hfd -nk 002965 | SxmlIndent | more
Pour mettre un lien sur cette page dans le réseau Wicri
{{Explor lien
|wiki= Wicri/Canada
|area= ParkinsonCanadaV1
|flux= Istex
|étape= Curation
|type= RBID
|clé= ISTEX:BB8F3730ECC8DBD4A3D2CD1FA4F55F29D184FA5C
|texte= Timing observations of rotating radio transients
}}
| This area was generated with Dilib version V0.6.29. |  |