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Discovery of gamma- and X-ray pulsations from the young and energetic PSR J1357-6429 with Fermi and XMM-Newton

Identifieur interne : 006B88 ( Main/Exploration ); précédent : 006B87; suivant : 006B89

Discovery of gamma- and X-ray pulsations from the young and energetic PSR J1357-6429 with Fermi and XMM-Newton

Auteurs : M. Lemoine-Goumard [France] ; V. E. Zavlin [États-Unis] ; M.-H. Grondin [Allemagne] ; R. Shannon [Australie] ; D. A. Smith [France] ; M. Burgay [Italie] ; F. Camilo [États-Unis] ; J. Cohen- Tanugi [France] ; P. C. C. Freire [Allemagne] ; J. E. Grove [États-Unis] ; L. Guillemot [Allemagne] ; S. Johnston [Australie] ; M. Keith [Australie] ; M. Kramer [Allemagne, Royaume-Uni] ; R. N. Manchester [Australie] ; P. F. Michelson [États-Unis] ; D. Parent [États-Unis] ; A. Possenti [Italie] ; P. S. Ray [États-Unis] ; M. Renaud [France] ; S. E. Thorsett [États-Unis] ; P. Weltevrede [Royaume-Uni] ; M. T. Wolff [États-Unis]

Source :

RBID : Pascal:12-0012757

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English descriptors

Abstract

Context. Since the launch of the Fermi satellite, the number of known gamma-ray pulsars has increased tenfold. Most gamma-ray detected pulsars are young and energetic, and many are associated with TeV sources. PSR J 1357-6429 is a high spin-down power pulsar (E = 3.1 × 1036 erg s-1), discovered during the Parkes multibeam survey of the Galactic plane, with significant timing noise typical of very young pulsars. In the very-high-energy domain (E > 100 GeV), H.E.S.S. has reported the detection of the extended source HESS J 1356-645 (intrinsic Gaussian width of 12') whose centroid lies 7' from PSR J 1357-6429. Aims. We search for gamma- and X-ray pulsations from this pulsar, characterize the neutron star emission and explore the environment of PSR J 1357-6429. Methods. Using a rotational ephemeris obtained with 74 observations made with the Parkes telescope at 1.4 GHz, we phase-fold more than two years of gamma-ray data acquired by the Large Area Telescope on-board Fermi as well as those collected with XMM-Newton, and perform gamma-ray spectral modeling. Results. Significant gamma- and X-ray pulsations are detected from PSR J1357-6429. The light curve in both bands shows one broad peak. Gamma-ray spectral analysis of the pulsed emission suggests that it is well described by a simple power-law of index 1.5 ± 0.3stat ± 0.3syst with an exponential cut-off at 0.8 ± 0.3stat ± 0.3syst GeV and an integral photon flux above 100 MeV of (6.5 ± 1.6stat ± 2.3sysc) x 10-8 cm-2 s-1. The X-ray spectra obtained from the new data provide results consistent with previous work. Upper limits on the gamma-ray emission from its potential pulsar wind nebula (PWN) are also reported. Conclusions. Assuming a distance of 2.4 kpc, the Fermi LAT energy flux yields a gamma-ray luminosity for PSR J1357-6429 of Lγ = (2.13 ± 0.25stat ± 0.83syst) x 1034 erg s-1, consistent with an Lγ √E========dot; relationship. The Fermi non-detection of the pulsar wind nebula associated with HESS J 1356-645 provides new constraints on the electron population responsible for the extended TeV emission.


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<title xml:lang="en" level="a">Discovery of gamma- and X-ray pulsations from the young and energetic PSR J1357-6429 with Fermi and XMM-Newton</title>
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<settlement type="city">Bonn</settlement>
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<wicri:noRegion>Epping NSW 1710</wicri:noRegion>
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<s1>CSIRO Astronomy and Space Science, Australia Telescope National Facility</s1>
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<wicri:noRegion>Epping NSW 1710</wicri:noRegion>
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<name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name>
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<inist:fA14 i1="08">
<s1>Max-Planck-Institut fur Radioastronomie, Auf dem Hügel 69</s1>
<s2>53121 Bonn</s2>
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<sZ>9 aut.</sZ>
<sZ>11 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>
</placeName>
</affiliation>
<affiliation wicri:level="4">
<inist:fA14 i1="10">
<s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
<s3>GBR</s3>
<sZ>14 aut.</sZ>
<sZ>22 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>
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<name sortKey="Manchester, R N" sort="Manchester, R N" uniqKey="Manchester R" first="R. N." last="Manchester">R. N. Manchester</name>
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<country>Australie</country>
<wicri:noRegion>Epping NSW 1710</wicri:noRegion>
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<name sortKey="Michelson, P F" sort="Michelson, P F" uniqKey="Michelson P" first="P. F." last="Michelson">P. F. Michelson</name>
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<inist:fA14 i1="11">
<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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<s3>USA</s3>
<sZ>16 aut.</sZ>
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<wicri:noRegion>Stanford, CA 94305</wicri:noRegion>
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<inist:fA14 i1="12">
<s1>Center for Earth Observing and Space Research, College of Science, George Mason University, Fairfax, VA 22030, resident at Naval Research Laboratory</s1>
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<sZ>17 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Washington, DC 20375</wicri:noRegion>
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<name sortKey="Possenti, A" sort="Possenti, A" uniqKey="Possenti A" first="A." last="Possenti">A. Possenti</name>
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<s1>INAF - Cagliari Astronomical Observatory</s1>
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<sZ>18 aut.</sZ>
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<country>Italie</country>
<wicri:noRegion>INAF - Cagliari Astronomical Observatory</wicri:noRegion>
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<name sortKey="Ray, P S" sort="Ray, P S" uniqKey="Ray P" first="P. S." last="Ray">P. S. Ray</name>
<affiliation wicri:level="1">
<inist:fA14 i1="09">
<s1>High Energy Space Environment Branch, Naval Research Laboratory</s1>
<s2>Washington, DC 20375</s2>
<s3>USA</s3>
<sZ>10 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>23 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Washington, DC 20375</wicri:noRegion>
</affiliation>
</author>
<author>
<name sortKey="Renaud, M" sort="Renaud, M" uniqKey="Renaud M" first="M." last="Renaud">M. Renaud</name>
<affiliation wicri:level="3">
<inist:fA14 i1="07">
<s1>Laboratoire Univers et Particules de Montpellier, Université Montpellier 2, CNRS/IN2P3</s1>
<s2>Montpellier</s2>
<s3>FRA</s3>
<sZ>8 aut.</sZ>
<sZ>20 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName>
<region type="region">Occitanie (région administrative)</region>
<region type="old region">Languedoc-Roussillon</region>
<settlement type="city">Montpellier</settlement>
</placeName>
</affiliation>
</author>
<author>
<name sortKey="Thorsett, S E" sort="Thorsett, S E" uniqKey="Thorsett S" first="S. E." last="Thorsett">S. E. Thorsett</name>
<affiliation wicri:level="1">
<inist:fA14 i1="13">
<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>21 aut.</sZ>
</inist:fA14>
<country>États-Unis</country>
<wicri:noRegion>Santa Cruz, CA 95064</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="10">
<s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
<s3>GBR</s3>
<sZ>14 aut.</sZ>
<sZ>22 aut.</sZ>
</inist:fA14>
<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="Wolff, M T" sort="Wolff, M T" uniqKey="Wolff M" first="M. T." last="Wolff">M. T. Wolff</name>
<affiliation wicri:level="1">
<inist:fA14 i1="09">
<s1>High Energy Space Environment Branch, Naval Research Laboratory</s1>
<s2>Washington, DC 20375</s2>
<s3>USA</s3>
<sZ>10 aut.</sZ>
<sZ>19 aut.</sZ>
<sZ>23 aut.</sZ>
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<country>États-Unis</country>
<wicri:noRegion>Washington, DC 20375</wicri:noRegion>
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</author>
</analytic>
<series>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
<imprint>
<date when="2011">2011</date>
</imprint>
</series>
</biblStruct>
</sourceDesc>
<seriesStmt>
<title level="j" type="main">Astronomy and astrophysics : (Berlin. Print)</title>
<title level="j" type="abbreviated">Astron. astrophys. : (Berl., Print)</title>
<idno type="ISSN">0004-6361</idno>
</seriesStmt>
</fileDesc>
<profileDesc>
<textClass>
<keywords scheme="KwdEn" xml:lang="en">
<term>Energetics</term>
<term>Energy transfer</term>
<term>Extended source</term>
<term>Fermi level</term>
<term>Galactic planes</term>
<term>Gamma emission</term>
<term>Gamma radiation</term>
<term>Light curves</term>
<term>Luminosity</term>
<term>Modelling</term>
<term>Neutron emission</term>
<term>Neutron stars</term>
<term>Power law</term>
<term>Pulsars</term>
<term>Spectral analysis</term>
<term>TeV range</term>
<term>Timing</term>
<term>Upper bound</term>
<term>Very high energy</term>
<term>X ray pulsation</term>
<term>X-ray spectra</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr">
<term>Rayonnement gamma</term>
<term>Pulsation RX</term>
<term>Energétique</term>
<term>Pulsar</term>
<term>Plan galactique</term>
<term>Timing</term>
<term>Très haute énergie</term>
<term>Source étendue</term>
<term>Etoile neutron</term>
<term>Emission neutron</term>
<term>Modélisation</term>
<term>Courbe lumière</term>
<term>Analyse spectrale</term>
<term>Loi puissance</term>
<term>Spectre RX</term>
<term>Borne supérieure</term>
<term>Emission gamma</term>
<term>Niveau Fermi</term>
<term>Transfert énergie</term>
<term>Luminosité</term>
<term>Domaine énergie TeV</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front>
<div type="abstract" xml:lang="en">Context. Since the launch of the Fermi satellite, the number of known gamma-ray pulsars has increased tenfold. Most gamma-ray detected pulsars are young and energetic, and many are associated with TeV sources. PSR J 1357-6429 is a high spin-down power pulsar (E = 3.1 × 10
<sup>36</sup>
erg s
<sup>-1</sup>
), discovered during the Parkes multibeam survey of the Galactic plane, with significant timing noise typical of very young pulsars. In the very-high-energy domain (E > 100 GeV), H.E.S.S. has reported the detection of the extended source HESS J 1356-645 (intrinsic Gaussian width of 12') whose centroid lies 7' from PSR J 1357-6429. Aims. We search for gamma- and X-ray pulsations from this pulsar, characterize the neutron star emission and explore the environment of PSR J 1357-6429. Methods. Using a rotational ephemeris obtained with 74 observations made with the Parkes telescope at 1.4 GHz, we phase-fold more than two years of gamma-ray data acquired by the Large Area Telescope on-board Fermi as well as those collected with XMM-Newton, and perform gamma-ray spectral modeling. Results. Significant gamma- and X-ray pulsations are detected from PSR J1357-6429. The light curve in both bands shows one broad peak. Gamma-ray spectral analysis of the pulsed emission suggests that it is well described by a simple power-law of index 1.5 ± 0.3
<sub>stat</sub>
± 0.3
<sub>syst</sub>
with an exponential cut-off at 0.8 ± 0.3
<sub>stat</sub>
± 0.3
<sub>syst</sub>
GeV and an integral photon flux above 100 MeV of (6.5 ± 1.6
<sub>stat</sub>
± 2.3
<sub>sysc</sub>
) x 10
<sup>-8</sup>
cm
<sup>-</sup>
2 s
<sup>-1</sup>
. The X-ray spectra obtained from the new data provide results consistent with previous work. Upper limits on the gamma-ray emission from its potential pulsar wind nebula (PWN) are also reported. Conclusions. Assuming a distance of 2.4 kpc, the Fermi LAT energy flux yields a gamma-ray luminosity for PSR J1357-6429 of L
<sub>γ</sub>
= (2.13 ± 0.25
<sub>stat</sub>
± 0.83
<sub>syst</sub>
) x 10
<sup>34</sup>
erg s
<sup>-1</sup>
, consistent with an Lγ √E========dot; relationship. The Fermi non-detection of the pulsar wind nebula associated with HESS J 1356-645 provides new constraints on the electron population responsible for the extended TeV emission.</div>
</front>
</TEI>
<affiliations>
<list>
<country>
<li>Allemagne</li>
<li>Australie</li>
<li>France</li>
<li>Italie</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region>
<li>Angleterre</li>
<li>Aquitaine</li>
<li>District de Cologne</li>
<li>Grand Manchester</li>
<li>Languedoc-Roussillon</li>
<li>Nouvelle-Aquitaine</li>
<li>Occitanie (région administrative)</li>
<li>Rhénanie-du-Nord-Westphalie</li>
<li>État de New York</li>
</region>
<settlement>
<li>Bonn</li>
<li>Gradignan</li>
<li>Manchester</li>
<li>Montpellier</li>
<li>New York</li>
</settlement>
<orgName>
<li>Université Columbia</li>
<li>Université de Manchester</li>
</orgName>
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<name sortKey="Lemoine Goumard, M" sort="Lemoine Goumard, M" uniqKey="Lemoine Goumard M" first="M." last="Lemoine-Goumard">M. Lemoine-Goumard</name>
</region>
<name sortKey="Cohen Tanugi, J" sort="Cohen Tanugi, J" uniqKey="Cohen Tanugi J" first="J." last="Cohen- Tanugi">J. Cohen- Tanugi</name>
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<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
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<noRegion>
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</noRegion>
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<name sortKey="Grove, J E" sort="Grove, J E" uniqKey="Grove J" first="J. E." last="Grove">J. E. Grove</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="Ray, P S" sort="Ray, P S" uniqKey="Ray P" first="P. S." last="Ray">P. S. Ray</name>
<name sortKey="Thorsett, S E" sort="Thorsett, S E" uniqKey="Thorsett S" first="S. E." last="Thorsett">S. E. Thorsett</name>
<name sortKey="Wolff, M T" sort="Wolff, M T" uniqKey="Wolff M" first="M. T." last="Wolff">M. T. Wolff</name>
</country>
<country name="Allemagne">
<noRegion>
<name sortKey="Grondin, M H" sort="Grondin, M H" uniqKey="Grondin M" first="M.-H." last="Grondin">M.-H. Grondin</name>
</noRegion>
<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>
<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="Shannon, R" sort="Shannon, R" uniqKey="Shannon R" first="R." last="Shannon">R. Shannon</name>
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<name sortKey="Keith, M" sort="Keith, M" uniqKey="Keith M" first="M." last="Keith">M. Keith</name>
<name sortKey="Manchester, R N" sort="Manchester, R N" uniqKey="Manchester R" first="R. N." last="Manchester">R. N. Manchester</name>
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<region name="Angleterre">
<name sortKey="Kramer, M" sort="Kramer, M" uniqKey="Kramer M" first="M." last="Kramer">M. Kramer</name>
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<name sortKey="Weltevrede, P" sort="Weltevrede, P" uniqKey="Weltevrede P" first="P." last="Weltevrede">P. Weltevrede</name>
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   |texte=   Discovery of gamma- and X-ray pulsations from the young and energetic PSR J1357-6429 with Fermi and XMM-Newton
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