Fermi-LAT constraints on the pulsar wind nebula nature of HESS J1857+026
Identifieur interne : 005C53 ( Main/Exploration ); précédent : 005C52; suivant : 005C54Fermi-LAT constraints on the pulsar wind nebula nature of HESS J1857+026
Auteurs : R. Rousseau [France] ; M.-H. Grondin [Allemagne] ; A. Van Etten [États-Unis] ; M. Lemoine-Goumard [France] ; S. Bogdanov [États-Unis] ; J. W. T. Hessels [Pays-Bas] ; V. M. Kaspi [Canada] ; Z. Arzoumanian [États-Unis] ; F. Camilo [États-Unis] ; J. M. Casandjian [France] ; C. M. Espinoza [Royaume-Uni] ; S. Johnston [Australie] ; A. G. Lyne [Royaume-Uni] ; D. A. Smith [France] ; B. W. Stappers [Royaume-Uni] ; G. A. Caliandro [Espagne]Source :
- Astronomy and astrophysics : (Berlin. Print) [ 0004-6361 ] ; 2012.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
Abstract
Context. Since its launch, the Fermi satellite has firmly identified 5 pulsar wind nebulae plus a large number of candidates, all powered by young and energetic pulsars. HESS J1857+026 is a spatially extended γ-ray source detected by H.E.S.S. and classified as a possible pulsar wind nebula candidate powered by PSR J 1856+0245. Aims. We search for γ-ray pulsations from PSR J 1856+0245 and explore the characteristics of its associated pulsar wind nebula. Methods. Using a rotational ephemeris obtained from the Lovell telescope at Jodrell Bank Observatory at 1.5 GHz, we phase-fold 36 months of γ-ray data acquired by the Large Area Telescope (LAT) aboard Fermi. We also perform a complete γ-ray spectral and morphological analysis. Results. No γ-ray pulsations were detected from PSR J1856+0245. However, significant emission is detected at a position coincident with the TeV source HESS J1857+026. The γ-ray spectrum is well described by a simple power-law with a spectral index of Γ = 1.53 ± 0.11stat ± 0.55syst and an energy flux of G(0.1-100 GeV) = (2.71 ± 0.52stat ± 1.51syst) × 10-11 erg cm-2 s-1. The γ-ray luminosity is LγPWN(0.1-100 GeV) = (2.5 ± O.5stat ± 1.5syst) x 1035 (d / 9 kpc)2 erg s-1, assuming a distance of 9 kpc. This implies a γ-ray efficiency of ∼5% for E========dot; = 4.6 × 1036 erg s-1, in the range expected for pulsar wind nebulae. Detailed multi-wavelength modeling provides new constraints on its pulsar wind nebula nature.
Affiliations:
- Allemagne, Australie, Canada, Espagne, France, Pays-Bas, Royaume-Uni, États-Unis
- Angleterre, Aquitaine, Bade-Wurtemberg, Catalogne, District de Karlsruhe, Grand Manchester, Hollande-Septentrionale, Nouvelle-Aquitaine, Québec, État de New York, Île-de-France
- Amsterdam, Gif-sur-Yvette, Gradignan, Heidelberg, Manchester, Montréal, New York
- Université Columbia, Université McGill, Université d'Amsterdam, Université de Manchester
Links toward previous steps (curation, corpus...)
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Le document en format XML
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<sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Fermi-LAT constraints on the pulsar wind nebula nature of HESS J1857+026</title>
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<region type="state">État de New York</region>
</placeName>
<orgName type="university">Université Columbia</orgName>
</affiliation>
</author>
<author><name sortKey="Casandjian, J M" sort="Casandjian, J M" uniqKey="Casandjian J" first="J. M." last="Casandjian">J. M. Casandjian</name>
<affiliation wicri:level="3"><inist:fA14 i1="10"><s1>Laboratoire AIM, CEA-IRFU/CNRS/Universite Paris Diderot, Service d'Astrophysique, CEA Saclay</s1>
<s2>91191 Gif-sur-Yvette</s2>
<s3>FRA</s3>
<sZ>10 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName><region type="region" nuts="2">Île-de-France</region>
<settlement type="city">Gif-sur-Yvette</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Espinoza, C M" sort="Espinoza, C M" uniqKey="Espinoza C" first="C. M." last="Espinoza">C. M. Espinoza</name>
<affiliation wicri:level="4"><inist:fA14 i1="11"><s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 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="Johnston, S" sort="Johnston, S" uniqKey="Johnston S" first="S." last="Johnston">S. Johnston</name>
<affiliation wicri:level="1"><inist:fA14 i1="12"><s1>CSIRO Astronomy and Space Science, Australia Telescope National Facility</s1>
<s2>Epping NSW 1710</s2>
<s3>AUS</s3>
<sZ>12 aut.</sZ>
</inist:fA14>
<country>Australie</country>
<wicri:noRegion>Epping NSW 1710</wicri:noRegion>
</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 wicri:level="4"><inist:fA14 i1="11"><s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 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="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</name>
<affiliation wicri:level="3"><inist:fA14 i1="01"><s1>Centre d'Etudes Nucléaires de Bordeaux Gradignan, Université Bordeaux 1, CNRS/IN2p3</s1>
<s2>33175 Gradignan</s2>
<s3>FRA</s3>
<sZ>1 aut.</sZ>
<sZ>4 aut.</sZ>
<sZ>14 aut.</sZ>
</inist:fA14>
<country>France</country>
<placeName><region type="region" nuts="2">Nouvelle-Aquitaine</region>
<region type="old region" nuts="2">Aquitaine</region>
<settlement type="city">Gradignan</settlement>
</placeName>
</affiliation>
</author>
<author><name sortKey="Stappers, B W" sort="Stappers, B W" uniqKey="Stappers B" first="B. W." last="Stappers">B. W. Stappers</name>
<affiliation wicri:level="4"><inist:fA14 i1="11"><s1>Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, The University of Manchester</s1>
<s2>M13 9PL</s2>
<s3>GBR</s3>
<sZ>11 aut.</sZ>
<sZ>13 aut.</sZ>
<sZ>15 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="Caliandro, G A" sort="Caliandro, G A" uniqKey="Caliandro G" first="G. A." last="Caliandro">G. A. Caliandro</name>
<affiliation wicri:level="2"><inist:fA14 i1="13"><s1>Institut de Ciències de l'Espai (IEEE-CSIC), Campus UAB</s1>
<s2>08193 Barcelona</s2>
<s3>ESP</s3>
<sZ>16 aut.</sZ>
</inist:fA14>
<country>Espagne</country>
<placeName><region nuts="2" type="communauté">Catalogne</region>
</placeName>
</affiliation>
</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="2012">2012</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>Cosmic gamma sources</term>
<term>Energetics</term>
<term>Energy transfer</term>
<term>Extended γ ray source</term>
<term>Gamma radiation</term>
<term>Gamma spectra</term>
<term>Luminosity</term>
<term>Modelling</term>
<term>Positions</term>
<term>Power law</term>
<term>Pulsars</term>
<term>Spatial observatory</term>
<term>Spectral analysis</term>
<term>Spectral index</term>
</keywords>
<keywords scheme="Pascal" xml:lang="fr"><term>Pulsar</term>
<term>Observatoire spatial</term>
<term>Energétique</term>
<term>Source Rγ étendue</term>
<term>Analyse spectrale</term>
<term>Position</term>
<term>Spectre gamma</term>
<term>Loi puissance</term>
<term>Indice spectral</term>
<term>Transfert énergie</term>
<term>Luminosité</term>
<term>Modélisation</term>
<term>Rayonnement gamma</term>
<term>Source gamma cosmique</term>
</keywords>
</textClass>
</profileDesc>
</teiHeader>
<front><div type="abstract" xml:lang="en">Context. Since its launch, the Fermi satellite has firmly identified 5 pulsar wind nebulae plus a large number of candidates, all powered by young and energetic pulsars. HESS J1857+026 is a spatially extended γ-ray source detected by H.E.S.S. and classified as a possible pulsar wind nebula candidate powered by PSR J 1856+0245. Aims. We search for γ-ray pulsations from PSR J 1856+0245 and explore the characteristics of its associated pulsar wind nebula. Methods. Using a rotational ephemeris obtained from the Lovell telescope at Jodrell Bank Observatory at 1.5 GHz, we phase-fold 36 months of γ-ray data acquired by the Large Area Telescope (LAT) aboard Fermi. We also perform a complete γ-ray spectral and morphological analysis. Results. No γ-ray pulsations were detected from PSR J1856+0245. However, significant emission is detected at a position coincident with the TeV source HESS J1857+026. The γ-ray spectrum is well described by a simple power-law with a spectral index of Γ = 1.53 ± 0.11<sub>stat</sub>
± 0.55<sub>syst</sub>
and an energy flux of G(0.1-100 GeV) = (2.71 ± 0.52<sub>stat</sub>
± 1.51<sub>syst</sub>
)<sub> </sub>
× 10<sup>-11</sup>
erg cm<sup>-2</sup>
s<sup>-1</sup>
. The γ-ray luminosity is L<sup>γ</sup>
<sub>PWN</sub>
(0.1-100 GeV) = (2.5 ± O.5<sub>stat</sub>
± 1.5<sub>s</sub>
y<sub>st</sub>
) x 10<sup>35</sup>
(d / 9 kpc)<sup>2</sup>
erg s<sup>-1</sup>
, assuming a distance of 9 kpc. This implies a γ-ray efficiency of ∼5% for E========dot; = 4.6 × 10<sup>36</sup>
erg s<sup>-1</sup>
, in the range expected for pulsar wind nebulae. Detailed multi-wavelength modeling provides new constraints on its pulsar wind nebula nature.</div>
</front>
</TEI>
<affiliations><list><country><li>Allemagne</li>
<li>Australie</li>
<li>Canada</li>
<li>Espagne</li>
<li>France</li>
<li>Pays-Bas</li>
<li>Royaume-Uni</li>
<li>États-Unis</li>
</country>
<region><li>Angleterre</li>
<li>Aquitaine</li>
<li>Bade-Wurtemberg</li>
<li>Catalogne</li>
<li>District de Karlsruhe</li>
<li>Grand Manchester</li>
<li>Hollande-Septentrionale</li>
<li>Nouvelle-Aquitaine</li>
<li>Québec</li>
<li>État de New York</li>
<li>Île-de-France</li>
</region>
<settlement><li>Amsterdam</li>
<li>Gif-sur-Yvette</li>
<li>Gradignan</li>
<li>Heidelberg</li>
<li>Manchester</li>
<li>Montréal</li>
<li>New York</li>
</settlement>
<orgName><li>Université Columbia</li>
<li>Université McGill</li>
<li>Université d'Amsterdam</li>
<li>Université de Manchester</li>
</orgName>
</list>
<tree><country name="France"><region name="Nouvelle-Aquitaine"><name sortKey="Rousseau, R" sort="Rousseau, R" uniqKey="Rousseau R" first="R." last="Rousseau">R. Rousseau</name>
</region>
<name sortKey="Casandjian, J M" sort="Casandjian, J M" uniqKey="Casandjian J" first="J. M." last="Casandjian">J. M. Casandjian</name>
<name sortKey="Lemoine Goumard, M" sort="Lemoine Goumard, M" uniqKey="Lemoine Goumard M" first="M." last="Lemoine-Goumard">M. Lemoine-Goumard</name>
<name sortKey="Smith, D A" sort="Smith, D A" uniqKey="Smith D" first="D. A." last="Smith">D. A. Smith</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="Grondin, M H" sort="Grondin, M H" uniqKey="Grondin M" first="M.-H." last="Grondin">M.-H. Grondin</name>
</country>
<country name="États-Unis"><noRegion><name sortKey="Van Etten, A" sort="Van Etten, A" uniqKey="Van Etten A" first="A." last="Van Etten">A. Van Etten</name>
</noRegion>
<name sortKey="Arzoumanian, Z" sort="Arzoumanian, Z" uniqKey="Arzoumanian Z" first="Z." last="Arzoumanian">Z. Arzoumanian</name>
<name sortKey="Bogdanov, S" sort="Bogdanov, S" uniqKey="Bogdanov S" first="S." last="Bogdanov">S. Bogdanov</name>
<name sortKey="Camilo, F" sort="Camilo, F" uniqKey="Camilo F" first="F." last="Camilo">F. Camilo</name>
</country>
<country name="Pays-Bas"><noRegion><name sortKey="Hessels, J W T" sort="Hessels, J W T" uniqKey="Hessels J" first="J. W. T." last="Hessels">J. W. T. Hessels</name>
</noRegion>
<name sortKey="Hessels, J W T" sort="Hessels, J W T" uniqKey="Hessels J" first="J. W. T." last="Hessels">J. W. T. Hessels</name>
</country>
<country name="Canada"><region name="Québec"><name sortKey="Kaspi, V M" sort="Kaspi, V M" uniqKey="Kaspi V" first="V. M." last="Kaspi">V. M. Kaspi</name>
</region>
</country>
<country name="Royaume-Uni"><region name="Angleterre"><name sortKey="Espinoza, C M" sort="Espinoza, C M" uniqKey="Espinoza C" first="C. M." last="Espinoza">C. M. Espinoza</name>
</region>
<name sortKey="Lyne, A G" sort="Lyne, A G" uniqKey="Lyne A" first="A. G." last="Lyne">A. G. Lyne</name>
<name sortKey="Stappers, B W" sort="Stappers, B W" uniqKey="Stappers B" first="B. W." last="Stappers">B. W. Stappers</name>
</country>
<country name="Australie"><noRegion><name sortKey="Johnston, S" sort="Johnston, S" uniqKey="Johnston S" first="S." last="Johnston">S. Johnston</name>
</noRegion>
</country>
<country name="Espagne"><region name="Catalogne"><name sortKey="Caliandro, G A" sort="Caliandro, G A" uniqKey="Caliandro G" first="G. A." last="Caliandro">G. A. Caliandro</name>
</region>
</country>
</tree>
</affiliations>
</record>
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