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THREE MILLISECOND PULSARS IN FERMI LAT UNASSOCIATED BRIGHT SOURCES

Identifieur interne : 006674 ( Main/Exploration ); précédent : 006673; suivant : 006675

THREE MILLISECOND PULSARS IN FERMI LAT UNASSOCIATED BRIGHT SOURCES

Auteurs : S. M. Ransom [États-Unis] ; P. S. Ray [États-Unis] ; F. Camilo [États-Unis] ; M. S. E. Roberts [États-Unis] ; Ö. Celik [États-Unis] ; M. T. Wolff [États-Unis] ; C. C. Cheung [États-Unis] ; M. Kerr [États-Unis] ; T. Pennucci [États-Unis] ; M. E. Decesar [États-Unis] ; I. Cognard [France] ; A. G. Lyne [Royaume-Uni] ; B. W. Stappers [Royaume-Uni] ; P. C. C. Freire [Allemagne] ; J. E. Grove [États-Unis] ; A. A. Abdo [États-Unis] ; G. Desvignes [États-Unis] ; D. Donato [États-Unis] ; E. C. Ferrara [États-Unis] ; N. Gehrels [États-Unis] ; L. Guillemot [Allemagne] ; C. Gwon [États-Unis] ; A. K. Harding [États-Unis] ; S. Johnston [Australie] ; M. Keith [Australie] ; M. Kramer [Royaume-Uni, Allemagne] ; P. F. Michelson [États-Unis] ; D. Parent [États-Unis] ; P. M. Saz Parkinson [États-Unis] ; R. W. Romani [États-Unis] ; D. A. Smith [France] ; G. Theureau [France] ; D. J. Thompson [États-Unis] ; P. Weltevrede [Royaume-Uni] ; K. S. Wood [États-Unis] ; M. Ziegler [États-Unis]

Source :

RBID : Pascal:11-0114593

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English descriptors

Abstract

We searched for radio pulsars in 25 of the non-variable, unassociated sources in the Fermi LAT Bright Source List with the Green Bank Telescope at 820 MHz. We report the discovery of three radio and γ-ray millisecond pulsars (MSPs) from a high Galactic latitude subset of these sources. All of the pulsars are in binary systems, which would have made them virtually impossible to detect in blind γ-ray pulsation searches. They seem to be relatively normal, nearby (≤2 kpc) MSPs. These observations, in combination with the Fermi detection of γ-rays from other known radio MSPs, imply that most, if not all, radio MSPs are efficient γ-ray producers. The γ-ray spectra of the pulsars are power law in nature with exponential cutoffs at a few GeV, as has been found with most other pulsars. The MSPs have all been detected as X-ray point sources. Their soft X-ray luminosities of ∼1030-1031 erg s-1 are typical of the rare radio MSPs seen in X-rays.


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<title xml:lang="en" level="a">THREE MILLISECOND PULSARS IN FERMI LAT UNASSOCIATED BRIGHT SOURCES</title>
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<settlement type="city">Manchester</settlement>
<region type="nation">Angleterre</region>
<region nuts="2" type="region">Grand Manchester</region>
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<s1>Max-Planck-Institut für Radioastronomie, Auf dem Hiigel 69</s1>
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<sZ>14 aut.</sZ>
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<country>Allemagne</country>
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<region type="land" nuts="1">Rhénanie-du-Nord-Westphalie</region>
<region type="district" nuts="2">District de Cologne</region>
<settlement type="city">Bonn</settlement>
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<s1>W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University</s1>
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<country>États-Unis</country>
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<s1>Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz</s1>
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<sZ>29 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
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<s1>W. W. Hansen Experimental Physics Laboratory, Kavli Institute for Particle Astrophysics and Cosmology, Department of Physics and SLAC National Accelerator Laboratory, Stanford University</s1>
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<country>États-Unis</country>
<wicri:noRegion>Stanford, CA 94305</wicri:noRegion>
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</author>
<author>
<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
<affiliation wicri:level="1">
<inist:fA14 i1="20">
<s1>Université Bordeaux 1, CNRS/IN2p3, Centre d'Études Nucléaires de Bordeaux Gradignan</s1>
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<s3>FRA</s3>
<sZ>31 aut.</sZ>
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<country>France</country>
<wicri:noRegion>33175 Gradignan</wicri:noRegion>
<wicri:noRegion>Centre d'Études Nucléaires de Bordeaux Gradignan</wicri:noRegion>
<wicri:noRegion>33175 Gradignan</wicri:noRegion>
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<name sortKey="Theureau, G" sort="Theureau, G" uniqKey="Theureau G" first="G." last="Theureau">G. Theureau</name>
<affiliation wicri:level="1">
<inist:fA14 i1="12">
<s1>Laboratoire de Physique et Chimie de l'Environnement, LPCE UMR 6115 CNRS, F-45071 Orléans Cedex 02, and Station de radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU</s1>
<s2>18330 Nançay</s2>
<s3>FRA</s3>
<sZ>11 aut.</sZ>
<sZ>32 aut.</sZ>
</inist:fA14>
<country>France</country>
<wicri:noRegion>18330 Nançay</wicri:noRegion>
<wicri:noRegion>CNRS/INSU</wicri:noRegion>
<wicri:noRegion>18330 Nançay</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Thompson, D J" sort="Thompson, D J" uniqKey="Thompson D" first="D. J." last="Thompson">D. J. Thompson</name>
<affiliation wicri:level="1">
<inist:fA14 i1="05">
<s1>NASA Goddard Space Flight Center</s1>
<s2>Greenbelt, MD 20771</s2>
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</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>NASA Goddard Space Flight Center</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Weltevrede, P" sort="Weltevrede, P" uniqKey="Weltevrede P" first="P." last="Weltevrede">P. Weltevrede</name>
<affiliation wicri:level="4">
<inist:fA14 i1="13">
<s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
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<sZ>12 aut.</sZ>
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<country>Royaume-Uni</country>
<placeName>
<settlement type="city">Manchester</settlement>
<region type="nation">Angleterre</region>
<region nuts="2" type="region">Grand Manchester</region>
</placeName>
<orgName type="university">Université de Manchester</orgName>
</affiliation>
</author>
<author>
<name sortKey="Wood, K S" sort="Wood, K S" uniqKey="Wood K" first="K. S." last="Wood">K. S. Wood</name>
<affiliation wicri:level="1">
<inist:fA14 i1="02">
<s1>Space Science Division, Naval Research Laboratory</s1>
<s2>Washington, DC 20375</s2>
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<sZ>2 aut.</sZ>
<sZ>6 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Washington, DC 20375</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Ziegler, M" sort="Ziegler, M" uniqKey="Ziegler M" first="M." last="Ziegler">M. Ziegler</name>
<affiliation wicri:level="1">
<inist:fA14 i1="19">
<s1>Santa Cruz Institute for Particle Physics, Department of Physics and Department of Astronomy and Astrophysics, University of California at Santa Cruz</s1>
<s2>Santa Cruz, CA 95064</s2>
<s3>USA</s3>
<sZ>29 aut.</sZ>
<sZ>36 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</wicri:noRegion>
</affiliation>
</author>
</analytic>
<series>
<title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
<imprint>
<date when="2011">2011</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">The Astrophysical journal</title>
<title level="j" type="abbreviated">Astrophys. j.</title>
<idno type="ISSN">0004-637X</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Gamma spectra</term>
<term>Luminosity</term>
<term>Millisecond pulsar</term>
<term>Point sources</term>
<term>Power law</term>
<term>Radiopulsar</term>
<term>Soft X radiation</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Pulsar milliseconde</term>
<term>Pulsar radio</term>
<term>Spectre gamma</term>
<term>Loi puissance</term>
<term>Source ponctuelle</term>
<term>Rayon X mou</term>
<term>Luminosité</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">We searched for radio pulsars in 25 of the non-variable, unassociated sources in the Fermi LAT Bright Source List with the Green Bank Telescope at 820 MHz. We report the discovery of three radio and γ-ray millisecond pulsars (MSPs) from a high Galactic latitude subset of these sources. All of the pulsars are in binary systems, which would have made them virtually impossible to detect in blind γ-ray pulsation searches. They seem to be relatively normal, nearby (≤2 kpc) MSPs. These observations, in combination with the Fermi detection of γ-rays from other known radio MSPs, imply that most, if not all, radio MSPs are efficient γ-ray producers. The γ-ray spectra of the pulsars are power law in nature with exponential cutoffs at a few GeV, as has been found with most other pulsars. The MSPs have all been detected as X-ray point sources. Their soft X-ray luminosities of ∼10
<sup>30</sup>
-10
<sup>31</sup>
erg s
<sup>-1</sup>
are typical of the rare radio MSPs seen in X-rays.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Allemagne</li>
<li>Australie</li>
<li>France</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Angleterre</li>
<li>Centre-Val de Loire</li>
<li>District de Cologne</li>
<li>Grand Manchester</li>
<li>Maryland</li>
<li>Rhénanie-du-Nord-Westphalie</li>
<li>Région Centre</li>
<li>État de New York</li>
</region>
<settlement>
<li>Bonn</li>
<li>College Park (Maryland)</li>
<li>Manchester</li>
<li>Nançay</li>
<li>New York</li>
</settlement>
<orgName>
<li>Université Columbia</li>
<li>Université de Manchester</li>
<li>Université du Maryland</li>
</orgName>
</list>
<tree>
<country name="États-Unis">
<noRegion>
<name sortKey="Ransom, S M" sort="Ransom, S M" uniqKey="Ransom S" first="S. M." last="Ransom">S. M. Ransom</name>
</noRegion>
<name sortKey="Abdo, A A" sort="Abdo, A A" uniqKey="Abdo A" first="A. A." last="Abdo">A. A. Abdo</name>
<name sortKey="Camilo, F" sort="Camilo, F" uniqKey="Camilo F" first="F." last="Camilo">F. Camilo</name>
<name sortKey="Celik, O" sort="Celik, O" uniqKey="Celik O" first="Ö." last="Celik">Ö. Celik</name>
<name sortKey="Celik, O" sort="Celik, O" uniqKey="Celik O" first="Ö." last="Celik">Ö. Celik</name>
<name sortKey="Celik, O" sort="Celik, O" uniqKey="Celik O" first="Ö." last="Celik">Ö. Celik</name>
<name sortKey="Cheung, C C" sort="Cheung, C C" uniqKey="Cheung C" first="C. C." last="Cheung">C. C. Cheung</name>
<name sortKey="Decesar, M E" sort="Decesar, M E" uniqKey="Decesar M" first="M. E." last="Decesar">M. E. Decesar</name>
<name sortKey="Decesar, M E" sort="Decesar, M E" uniqKey="Decesar M" first="M. E." last="Decesar">M. E. Decesar</name>
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<name sortKey="Desvignes, G" sort="Desvignes, G" uniqKey="Desvignes G" first="G." last="Desvignes">G. Desvignes</name>
<name sortKey="Donato, D" sort="Donato, D" uniqKey="Donato D" first="D." last="Donato">D. Donato</name>
<name sortKey="Donato, D" sort="Donato, D" uniqKey="Donato D" first="D." last="Donato">D. Donato</name>
<name sortKey="Ferrara, E C" sort="Ferrara, E C" uniqKey="Ferrara E" first="E. C." last="Ferrara">E. C. Ferrara</name>
<name sortKey="Gehrels, N" sort="Gehrels, N" uniqKey="Gehrels N" first="N." last="Gehrels">N. Gehrels</name>
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<name sortKey="Gwon, C" sort="Gwon, C" uniqKey="Gwon C" first="C." last="Gwon">C. Gwon</name>
<name sortKey="Harding, A K" sort="Harding, A K" uniqKey="Harding A" first="A. K." last="Harding">A. K. Harding</name>
<name sortKey="Kerr, M" sort="Kerr, M" uniqKey="Kerr M" first="M." last="Kerr">M. Kerr</name>
<name sortKey="Michelson, P F" sort="Michelson, P F" uniqKey="Michelson P" first="P. F." last="Michelson">P. F. Michelson</name>
<name sortKey="Parent, D" sort="Parent, D" uniqKey="Parent D" first="D." last="Parent">D. Parent</name>
<name sortKey="Pennucci, T" sort="Pennucci, T" uniqKey="Pennucci T" first="T." last="Pennucci">T. Pennucci</name>
<name sortKey="Ray, P S" sort="Ray, P S" uniqKey="Ray P" first="P. S." last="Ray">P. S. Ray</name>
<name sortKey="Roberts, M S E" sort="Roberts, M S E" uniqKey="Roberts M" first="M. S. E." last="Roberts">M. S. E. Roberts</name>
<name sortKey="Romani, R W" sort="Romani, R W" uniqKey="Romani R" first="R. W." last="Romani">R. W. Romani</name>
<name sortKey="Saz Parkinson, P M" sort="Saz Parkinson, P M" uniqKey="Saz Parkinson P" first="P. M." last="Saz Parkinson">P. M. Saz Parkinson</name>
<name sortKey="Thompson, D J" sort="Thompson, D J" uniqKey="Thompson D" first="D. J." last="Thompson">D. J. Thompson</name>
<name sortKey="Wolff, M T" sort="Wolff, M T" uniqKey="Wolff M" first="M. T." last="Wolff">M. T. Wolff</name>
<name sortKey="Wood, K S" sort="Wood, K S" uniqKey="Wood K" first="K. S." last="Wood">K. S. Wood</name>
<name sortKey="Ziegler, M" sort="Ziegler, M" uniqKey="Ziegler M" first="M." last="Ziegler">M. Ziegler</name>
</country>
<country name="France">
<region name="Centre-Val de Loire">
<name sortKey="Cognard, I" sort="Cognard, I" uniqKey="Cognard I" first="I." last="Cognard">I. Cognard</name>
</region>
<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
<name sortKey="Theureau, G" sort="Theureau, G" uniqKey="Theureau G" first="G." last="Theureau">G. Theureau</name>
</country>
<country name="Royaume-Uni">
<region name="Angleterre">
<name sortKey="Lyne, A G" sort="Lyne, A G" uniqKey="Lyne A" first="A. G." last="Lyne">A. G. Lyne</name>
</region>
<name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name>
<name sortKey="Stappers, B W" sort="Stappers, B W" uniqKey="Stappers B" first="B. W." last="Stappers">B. W. Stappers</name>
<name sortKey="Weltevrede, P" sort="Weltevrede, P" uniqKey="Weltevrede P" first="P." last="Weltevrede">P. Weltevrede</name>
</country>
<country name="Allemagne">
<region name="Rhénanie-du-Nord-Westphalie">
<name sortKey="Freire, P C C" sort="Freire, P C C" uniqKey="Freire P" first="P. C. C." last="Freire">P. C. C. Freire</name>
</region>
<name sortKey="Guillemot, L" sort="Guillemot, L" uniqKey="Guillemot L" first="L." last="Guillemot">L. Guillemot</name>
<name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name>
</country>
<country name="Australie">
<noRegion>
<name sortKey="Johnston, S" sort="Johnston, S" uniqKey="Johnston S" first="S." last="Johnston">S. Johnston</name>
</noRegion>
<name sortKey="Keith, M" sort="Keith, M" uniqKey="Keith M" first="M." last="Keith">M. Keith</name>
</country>
</tree>
</affiliations>
</record>

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   |area=    AustralieFrV1
   |flux=    Main
   |étape=   Exploration
   |type=    RBID
   |clé=     Pascal:11-0114593
   |texte=   THREE MILLISECOND PULSARS IN FERMI LAT UNASSOCIATED BRIGHT SOURCES
}}

Wicri

This area was generated with Dilib version V0.6.33.
Data generation: Tue Dec 5 10:43:12 2017. Site generation: Tue Mar 5 14:07:20 2024