A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223
Identifieur interne : 004831 ( PascalFrancis/Curation ); précédent : 004830; suivant : 004832A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223
Auteurs : D. M. Russell [Pays-Bas] ; P. A. Curran [France] ; T. Munoz-Darias [Italie] ; F. Lewis [Royaume-Uni] ; S. Motta [Italie] ; H. Stiele [Italie] ; T. Belloni [Italie] ; J. C. A. Miller-Jones [Australie] ; P. G. Jonker [Pays-Bas, États-Unis] ; K. O'Brien [États-Unis] ; J. Homan [États-Unis] ; P. Casella [Royaume-Uni] ; P. Gandhi [Japon] ; P. Soleri [Pays-Bas] ; S. Markoff [Pays-Bas] ; D. Maitra [États-Unis] ; E. Gallo [États-Unis] ; M. Cadolle Bel [Espagne]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2012.
Descripteurs français
- Pascal (Inist)
- Jet, Trou noir, Quiescence, Courbe lumière, Emission optique, Sursaut optique, Densité spectrale énergie, Morphologie, Photométrie IR, Polarimétrie, Borne supérieure, Polarisation rectiligne, Indice spectral, Déplacement fréquence, Accrétion, Disque accrétion, Binaire RX, Source RX binaire, Cosmologie, Source RX cosmique.
- Wicri :
- topic : Cosmologie.
English descriptors
- KwdEn :
- Accretion, Accretion disks, Binary X ray source, Black holes, Cosmic x-ray sources, Cosmology, Frequency shift, Infrared photometry, Jets, Light curves, Light emission, Linear polarization, Morphology, Optical burst, Polarimetry, Quiescence, Spectral energy distribution, Spectral index, Upper bound, X-ray binary stars.
Abstract
We present optical monitoring of the black hole candidate XTE J1752-223 during its 2009-10 outburst and decay to quiescence. The optical light curve can be described by an exponential decay followed by a plateau, then a more rapid fade towards quiescence. The plateau appears to be due to an extra component of optical emission that brightens and then fades over ∼40 days. We show evidence for the origin of this optical 'flare' to be the synchrotron jet during the decaying hard state, and we identify and isolate both disc and jet components in the spectral energy distributions. The optical flare has the same morphology and amplitude as a contemporaneous X-ray rebrightening. This suggests a common origin, but no firm conclusions can be made favouring or disfavouring the jet producing the X-ray flare. The quiescent optical magnitudes are B ≥ 20.6, V ≥ 21.1, R ≥ 19.5, i' ≥ 19.2. From the optical outburst amplitude we estimate a likely orbital period of <22 h. We also present near-infrared (NIR) photometry and polarimetry and rare mid-IR imaging (8-12 μm) when the source is nearing quiescence. The fading jet component, and possibly the companion star, may contribute to the NIR flux. We derive deep mid-IR flux upper limits and NIR linear polarization upper limits. With the inclusion of radio data, we measure an almost flat jet spectral index between radio and optical; Fν ν∼+0.05. The data favour the jet break to optically thin emission to reside in the IR, but may shift to frequencies as high as the optical or UV during the peak of the flare.
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<record><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223</title><author><name sortKey="Russell, D M" sort="Russell, D M" uniqKey="Russell D" first="D. M." last="Russell">D. M. Russell</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, PO Box 94249</s1><s2>1090 GE Amsterdam</s2><s3>NLD</s3><sZ>1 aut.</sZ><sZ>15 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Curran, P A" sort="Curran, P A" uniqKey="Curran P" first="P. A." last="Curran">P. A. Curran</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Laboratoire AIM, CEA/IRFU-Université Paris Diderot-CNRS/INSU, CEA DSM/IRFU/SAp, Centre de Saclay</s1><s2>91191 Gif-sur-Yvette</s2><s3>FRA</s3><sZ>2 aut.</sZ></inist:fA14><country>France</country></affiliation></author><author><name sortKey="Munoz Darias, T" sort="Munoz Darias, T" uniqKey="Munoz Darias T" first="T." last="Munoz-Darias">T. Munoz-Darias</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Lewis, F" sort="Lewis, F" uniqKey="Lewis F" first="F." last="Lewis">F. Lewis</name><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Faulkes Telescope Project, University of Glamorgan</s1><s2>Pontypridd CF37 1DL</s2><s3>GBR</s3><sZ>4 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Department of Physics and Astronomy, The Open Universiy, Walton Hall</s1><s2>Milton Keynes MK7 6AA</s2><s3>GBR</s3><sZ>4 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation></author><author><name sortKey="Motta, S" sort="Motta, S" uniqKey="Motta S" first="S." last="Motta">S. Motta</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Stiele, H" sort="Stiele, H" uniqKey="Stiele H" first="H." last="Stiele">H. Stiele</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Belloni, T" sort="Belloni, T" uniqKey="Belloni T" first="T." last="Belloni">T. Belloni</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Miller Jones, J C A" sort="Miller Jones, J C A" uniqKey="Miller Jones J" first="J. C. A." last="Miller-Jones">J. C. A. Miller-Jones</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987</s1><s2>Perth, WA 6845</s2><s3>AUS</s3><sZ>8 aut.</sZ></inist:fA14><country>Australie</country></affiliation></author><author><name sortKey="Jonker, P G" sort="Jonker, P G" uniqKey="Jonker P" first="P. G." last="Jonker">P. G. Jonker</name><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>SRON, Netherlands Institute for Space Research, Sorbonnelaan 2</s1><s2>3584 CA, Utrecht</s2><s3>NLD</s3><sZ>9 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Harvard-Smithsonian Center for Astrophysics, 60 Garden Street</s1><s2>Cambridge, MA 02138</s2><s3>USA</s3><sZ>9 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="09"><s1>Department of Astraphysics, IMAPP, Radboud University Nijmegen, PO Box 9010</s1><s2>6500 GL Nijmegen</s2><s3>NLD</s3><sZ>9 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="O Brien, K" sort="O Brien, K" uniqKey="O Brien K" first="K." last="O'Brien">K. O'Brien</name><affiliation wicri:level="1"><inist:fA14 i1="10"><s1>Department of Physics, University of California</s1><s2>Santa Barbara, CA 93106-9530</s2><s3>USA</s3><sZ>10 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Homan, J" sort="Homan, J" uniqKey="Homan J" first="J." last="Homan">J. Homan</name><affiliation wicri:level="1"><inist:fA14 i1="11"><s1>MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street</s1><s2>Cambridge, MA 02139</s2><s3>USA</s3><sZ>11 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Casella, P" sort="Casella, P" uniqKey="Casella P" first="P." last="Casella">P. Casella</name><affiliation wicri:level="1"><inist:fA14 i1="12"><s1>School of Physics and Astronomy, University of Southampton</s1><s2>Southampton, Hampshire SO17 IBJ</s2><s3>GBR</s3><sZ>12 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation></author><author><name sortKey="Gandhi, P" sort="Gandhi, P" uniqKey="Gandhi P" first="P." last="Gandhi">P. Gandhi</name><affiliation wicri:level="1"><inist:fA14 i1="13"><s1>ISAS, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, chuo-ku</s1><s2>Sngamihara, Kanagawa 229-8510</s2><s3>JPN</s3><sZ>13 aut.</sZ></inist:fA14><country>Japon</country></affiliation></author><author><name sortKey="Soleri, P" sort="Soleri, P" uniqKey="Soleri P" first="P." last="Soleri">P. Soleri</name><affiliation wicri:level="1"><inist:fA14 i1="14"><s1>Kapteyn Astronomical Institute, University of Groningen, PO Box 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>14 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Markoff, S" sort="Markoff, S" uniqKey="Markoff S" first="S." last="Markoff">S. Markoff</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, PO Box 94249</s1><s2>1090 GE Amsterdam</s2><s3>NLD</s3><sZ>1 aut.</sZ><sZ>15 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Maitra, D" sort="Maitra, D" uniqKey="Maitra D" first="D." last="Maitra">D. Maitra</name><affiliation wicri:level="1"><inist:fA14 i1="15"><s1>Department of Astronomy, University of Michigan, 500 Church Street</s1><s2>Ann Arbor, MI 48109</s2><s3>USA</s3><sZ>16 aut.</sZ><sZ>17 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Gallo, E" sort="Gallo, E" uniqKey="Gallo E" first="E." last="Gallo">E. Gallo</name><affiliation wicri:level="1"><inist:fA14 i1="15"><s1>Department of Astronomy, University of Michigan, 500 Church Street</s1><s2>Ann Arbor, MI 48109</s2><s3>USA</s3><sZ>16 aut.</sZ><sZ>17 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Cadolle Bel, M" sort="Cadolle Bel, M" uniqKey="Cadolle Bel M" first="M." last="Cadolle Bel">M. Cadolle Bel</name><affiliation wicri:level="1"><inist:fA14 i1="16"><s1>ESAC, ISOC, Villanueva de la Canada, Madrid P. O. Box 78</s1><s2>28691</s2><s3>ESP</s3><sZ>18 aut.</sZ></inist:fA14><country>Espagne</country></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">12-0042281</idno><date when="2012">2012</date><idno type="stanalyst">PASCAL 12-0042281 INIST</idno><idno type="RBID">Pascal:12-0042281</idno><idno type="wicri:Area/PascalFrancis/Corpus">001679</idno><idno type="wicri:Area/PascalFrancis/Curation">004831</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223</title><author><name sortKey="Russell, D M" sort="Russell, D M" uniqKey="Russell D" first="D. M." last="Russell">D. M. Russell</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, PO Box 94249</s1><s2>1090 GE Amsterdam</s2><s3>NLD</s3><sZ>1 aut.</sZ><sZ>15 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Curran, P A" sort="Curran, P A" uniqKey="Curran P" first="P. A." last="Curran">P. A. Curran</name><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>Laboratoire AIM, CEA/IRFU-Université Paris Diderot-CNRS/INSU, CEA DSM/IRFU/SAp, Centre de Saclay</s1><s2>91191 Gif-sur-Yvette</s2><s3>FRA</s3><sZ>2 aut.</sZ></inist:fA14><country>France</country></affiliation></author><author><name sortKey="Munoz Darias, T" sort="Munoz Darias, T" uniqKey="Munoz Darias T" first="T." last="Munoz-Darias">T. Munoz-Darias</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Lewis, F" sort="Lewis, F" uniqKey="Lewis F" first="F." last="Lewis">F. Lewis</name><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Faulkes Telescope Project, University of Glamorgan</s1><s2>Pontypridd CF37 1DL</s2><s3>GBR</s3><sZ>4 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Department of Physics and Astronomy, The Open Universiy, Walton Hall</s1><s2>Milton Keynes MK7 6AA</s2><s3>GBR</s3><sZ>4 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation></author><author><name sortKey="Motta, S" sort="Motta, S" uniqKey="Motta S" first="S." last="Motta">S. Motta</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Stiele, H" sort="Stiele, H" uniqKey="Stiele H" first="H." last="Stiele">H. Stiele</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Belloni, T" sort="Belloni, T" uniqKey="Belloni T" first="T." last="Belloni">T. Belloni</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></inist:fA14><country>Italie</country></affiliation></author><author><name sortKey="Miller Jones, J C A" sort="Miller Jones, J C A" uniqKey="Miller Jones J" first="J. C. A." last="Miller-Jones">J. C. A. Miller-Jones</name><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987</s1><s2>Perth, WA 6845</s2><s3>AUS</s3><sZ>8 aut.</sZ></inist:fA14><country>Australie</country></affiliation></author><author><name sortKey="Jonker, P G" sort="Jonker, P G" uniqKey="Jonker P" first="P. G." last="Jonker">P. G. Jonker</name><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>SRON, Netherlands Institute for Space Research, Sorbonnelaan 2</s1><s2>3584 CA, Utrecht</s2><s3>NLD</s3><sZ>9 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="08"><s1>Harvard-Smithsonian Center for Astrophysics, 60 Garden Street</s1><s2>Cambridge, MA 02138</s2><s3>USA</s3><sZ>9 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation><affiliation wicri:level="1"><inist:fA14 i1="09"><s1>Department of Astraphysics, IMAPP, Radboud University Nijmegen, PO Box 9010</s1><s2>6500 GL Nijmegen</s2><s3>NLD</s3><sZ>9 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="O Brien, K" sort="O Brien, K" uniqKey="O Brien K" first="K." last="O'Brien">K. O'Brien</name><affiliation wicri:level="1"><inist:fA14 i1="10"><s1>Department of Physics, University of California</s1><s2>Santa Barbara, CA 93106-9530</s2><s3>USA</s3><sZ>10 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Homan, J" sort="Homan, J" uniqKey="Homan J" first="J." last="Homan">J. Homan</name><affiliation wicri:level="1"><inist:fA14 i1="11"><s1>MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street</s1><s2>Cambridge, MA 02139</s2><s3>USA</s3><sZ>11 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Casella, P" sort="Casella, P" uniqKey="Casella P" first="P." last="Casella">P. Casella</name><affiliation wicri:level="1"><inist:fA14 i1="12"><s1>School of Physics and Astronomy, University of Southampton</s1><s2>Southampton, Hampshire SO17 IBJ</s2><s3>GBR</s3><sZ>12 aut.</sZ></inist:fA14><country>Royaume-Uni</country></affiliation></author><author><name sortKey="Gandhi, P" sort="Gandhi, P" uniqKey="Gandhi P" first="P." last="Gandhi">P. Gandhi</name><affiliation wicri:level="1"><inist:fA14 i1="13"><s1>ISAS, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, chuo-ku</s1><s2>Sngamihara, Kanagawa 229-8510</s2><s3>JPN</s3><sZ>13 aut.</sZ></inist:fA14><country>Japon</country></affiliation></author><author><name sortKey="Soleri, P" sort="Soleri, P" uniqKey="Soleri P" first="P." last="Soleri">P. Soleri</name><affiliation wicri:level="1"><inist:fA14 i1="14"><s1>Kapteyn Astronomical Institute, University of Groningen, PO Box 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>14 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Markoff, S" sort="Markoff, S" uniqKey="Markoff S" first="S." last="Markoff">S. Markoff</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, PO Box 94249</s1><s2>1090 GE Amsterdam</s2><s3>NLD</s3><sZ>1 aut.</sZ><sZ>15 aut.</sZ></inist:fA14><country>Pays-Bas</country></affiliation></author><author><name sortKey="Maitra, D" sort="Maitra, D" uniqKey="Maitra D" first="D." last="Maitra">D. Maitra</name><affiliation wicri:level="1"><inist:fA14 i1="15"><s1>Department of Astronomy, University of Michigan, 500 Church Street</s1><s2>Ann Arbor, MI 48109</s2><s3>USA</s3><sZ>16 aut.</sZ><sZ>17 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Gallo, E" sort="Gallo, E" uniqKey="Gallo E" first="E." last="Gallo">E. Gallo</name><affiliation wicri:level="1"><inist:fA14 i1="15"><s1>Department of Astronomy, University of Michigan, 500 Church Street</s1><s2>Ann Arbor, MI 48109</s2><s3>USA</s3><sZ>16 aut.</sZ><sZ>17 aut.</sZ></inist:fA14><country>États-Unis</country></affiliation></author><author><name sortKey="Cadolle Bel, M" sort="Cadolle Bel, M" uniqKey="Cadolle Bel M" first="M." last="Cadolle Bel">M. Cadolle Bel</name><affiliation wicri:level="1"><inist:fA14 i1="16"><s1>ESAC, ISOC, Villanueva de la Canada, Madrid P. O. Box 78</s1><s2>28691</s2><s3>ESP</s3><sZ>18 aut.</sZ></inist:fA14><country>Espagne</country></affiliation></author></analytic><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno><imprint><date when="2012">2012</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accretion</term><term>Accretion disks</term><term>Binary X ray source</term><term>Black holes</term><term>Cosmic x-ray sources</term><term>Cosmology</term><term>Frequency shift</term><term>Infrared photometry</term><term>Jets</term><term>Light curves</term><term>Light emission</term><term>Linear polarization</term><term>Morphology</term><term>Optical burst</term><term>Polarimetry</term><term>Quiescence</term><term>Spectral energy distribution</term><term>Spectral index</term><term>Upper bound</term><term>X-ray binary stars</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Jet</term><term>Trou noir</term><term>Quiescence</term><term>Courbe lumière</term><term>Emission optique</term><term>Sursaut optique</term><term>Densité spectrale énergie</term><term>Morphologie</term><term>Photométrie IR</term><term>Polarimétrie</term><term>Borne supérieure</term><term>Polarisation rectiligne</term><term>Indice spectral</term><term>Déplacement fréquence</term><term>Accrétion</term><term>Disque accrétion</term><term>Binaire RX</term><term>Source RX binaire</term><term>Cosmologie</term><term>Source RX cosmique</term></keywords><keywords scheme="Wicri" type="topic" xml:lang="fr"><term>Cosmologie</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">We present optical monitoring of the black hole candidate XTE J1752-223 during its 2009-10 outburst and decay to quiescence. The optical light curve can be described by an exponential decay followed by a plateau, then a more rapid fade towards quiescence. The plateau appears to be due to an extra component of optical emission that brightens and then fades over ∼40 days. We show evidence for the origin of this optical 'flare' to be the synchrotron jet during the decaying hard state, and we identify and isolate both disc and jet components in the spectral energy distributions. The optical flare has the same morphology and amplitude as a contemporaneous X-ray rebrightening. This suggests a common origin, but no firm conclusions can be made favouring or disfavouring the jet producing the X-ray flare. The quiescent optical magnitudes are B ≥ 20.6, V ≥ 21.1, R ≥ 19.5, i' ≥ 19.2. From the optical outburst amplitude we estimate a likely orbital period of <22 h. We also present near-infrared (NIR) photometry and polarimetry and rare mid-IR imaging (8-12 μm) when the source is nearing quiescence. The fading jet component, and possibly the companion star, may contribute to the NIR flux. We derive deep mid-IR flux upper limits and NIR linear polarization upper limits. With the inclusion of radio data, we measure an almost flat jet spectral index between radio and optical; F<sub>ν</sub> ν<sup>∼+0.05</sup>. The data favour the jet break to optically thin emission to reside in the IR, but may shift to frequencies as high as the optical or UV during the peak of the flare.</div> </front></TEI><inist><standard h6="B"><pA><fA01 i1="01" i2="1"><s0>0035-8711</s0></fA01><fA02 i1="01"><s0>MNRAA4</s0></fA02><fA03 i2="1"><s0>Mon. Not. R. Astron. Soc.</s0></fA03><fA05><s2>419</s2></fA05><fA06><s2>2</s2></fA06><fA08 i1="01" i2="1" l="ENG"><s1>A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223</s1></fA08><fA11 i1="01" i2="1"><s1>RUSSELL (D. M.)</s1></fA11><fA11 i1="02" i2="1"><s1>CURRAN (P. A.)</s1></fA11><fA11 i1="03" i2="1"><s1>MUNOZ-DARIAS (T.)</s1></fA11><fA11 i1="04" i2="1"><s1>LEWIS (F.)</s1></fA11><fA11 i1="05" i2="1"><s1>MOTTA (S.)</s1></fA11><fA11 i1="06" i2="1"><s1>STIELE (H.)</s1></fA11><fA11 i1="07" i2="1"><s1>BELLONI (T.)</s1></fA11><fA11 i1="08" i2="1"><s1>MILLER-JONES (J. C. A.)</s1></fA11><fA11 i1="09" i2="1"><s1>JONKER (P. G.)</s1></fA11><fA11 i1="10" i2="1"><s1>O'BRIEN (K.)</s1></fA11><fA11 i1="11" i2="1"><s1>HOMAN (J.)</s1></fA11><fA11 i1="12" i2="1"><s1>CASELLA (P.)</s1></fA11><fA11 i1="13" i2="1"><s1>GANDHI (P.)</s1></fA11><fA11 i1="14" i2="1"><s1>SOLERI (P.)</s1></fA11><fA11 i1="15" i2="1"><s1>MARKOFF (S.)</s1></fA11><fA11 i1="16" i2="1"><s1>MAITRA (D.)</s1></fA11><fA11 i1="17" i2="1"><s1>GALLO (E.)</s1></fA11><fA11 i1="18" i2="1"><s1>CADOLLE BEL (M.)</s1></fA11><fA14 i1="01"><s1>Astronomical Institute 'Anton Pannekoek', University of Amsterdam, PO Box 94249</s1><s2>1090 GE Amsterdam</s2><s3>NLD</s3><sZ>1 aut.</sZ><sZ>15 aut.</sZ></fA14><fA14 i1="02"><s1>Laboratoire AIM, CEA/IRFU-Université Paris Diderot-CNRS/INSU, CEA DSM/IRFU/SAp, Centre de Saclay</s1><s2>91191 Gif-sur-Yvette</s2><s3>FRA</s3><sZ>2 aut.</sZ></fA14><fA14 i1="03"><s1>INAF-Osservatorio Astronomico di Brera, Via E. Bianchi 46</s1><s2>23807 Merate (LC</s2><s3>ITA</s3><sZ>3 aut.</sZ><sZ>5 aut.</sZ><sZ>6 aut.</sZ><sZ>7 aut.</sZ></fA14><fA14 i1="04"><s1>Faulkes Telescope Project, University of Glamorgan</s1><s2>Pontypridd CF37 1DL</s2><s3>GBR</s3><sZ>4 aut.</sZ></fA14><fA14 i1="05"><s1>Department of Physics and Astronomy, The Open Universiy, Walton Hall</s1><s2>Milton Keynes MK7 6AA</s2><s3>GBR</s3><sZ>4 aut.</sZ></fA14><fA14 i1="06"><s1>International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987</s1><s2>Perth, WA 6845</s2><s3>AUS</s3><sZ>8 aut.</sZ></fA14><fA14 i1="07"><s1>SRON, Netherlands Institute for Space Research, Sorbonnelaan 2</s1><s2>3584 CA, Utrecht</s2><s3>NLD</s3><sZ>9 aut.</sZ></fA14><fA14 i1="08"><s1>Harvard-Smithsonian Center for Astrophysics, 60 Garden Street</s1><s2>Cambridge, MA 02138</s2><s3>USA</s3><sZ>9 aut.</sZ></fA14><fA14 i1="09"><s1>Department of Astraphysics, IMAPP, Radboud University Nijmegen, PO Box 9010</s1><s2>6500 GL Nijmegen</s2><s3>NLD</s3><sZ>9 aut.</sZ></fA14><fA14 i1="10"><s1>Department of Physics, University of California</s1><s2>Santa Barbara, CA 93106-9530</s2><s3>USA</s3><sZ>10 aut.</sZ></fA14><fA14 i1="11"><s1>MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street</s1><s2>Cambridge, MA 02139</s2><s3>USA</s3><sZ>11 aut.</sZ></fA14><fA14 i1="12"><s1>School of Physics and Astronomy, University of Southampton</s1><s2>Southampton, Hampshire SO17 IBJ</s2><s3>GBR</s3><sZ>12 aut.</sZ></fA14><fA14 i1="13"><s1>ISAS, Japan Aerospace Exploration Agency, 3-1-1 Yoshinodai, chuo-ku</s1><s2>Sngamihara, Kanagawa 229-8510</s2><s3>JPN</s3><sZ>13 aut.</sZ></fA14><fA14 i1="14"><s1>Kapteyn Astronomical Institute, University of Groningen, PO Box 800</s1><s2>9700 AV Groningen</s2><s3>NLD</s3><sZ>14 aut.</sZ></fA14><fA14 i1="15"><s1>Department of Astronomy, University of Michigan, 500 Church Street</s1><s2>Ann Arbor, MI 48109</s2><s3>USA</s3><sZ>16 aut.</sZ><sZ>17 aut.</sZ></fA14><fA14 i1="16"><s1>ESAC, ISOC, Villanueva de la Canada, Madrid P. O. Box 78</s1><s2>28691</s2><s3>ESP</s3><sZ>18 aut.</sZ></fA14><fA20><s1>1740-1751</s1></fA20><fA21><s1>2012</s1></fA21><fA23 i1="01"><s0>ENG</s0></fA23><fA43 i1="01"><s1>INIST</s1><s2>2067</s2><s5>354000506050220740</s5></fA43><fA44><s0>0000</s0><s1>© 2012 INIST-CNRS. All rights reserved.</s1></fA44><fA45><s0>1 p.1/4</s0></fA45><fA47 i1="01" i2="1"><s0>12-0042281</s0></fA47><fA60><s1>P</s1></fA60><fA61><s0>A</s0></fA61><fA64 i1="01" i2="1"><s0>Monthly Notices of the Royal Astronomical Society</s0></fA64><fA66 i1="01"><s0>USA</s0></fA66><fC01 i1="01" l="ENG"><s0>We present optical monitoring of the black hole candidate XTE J1752-223 during its 2009-10 outburst and decay to quiescence. The optical light curve can be described by an exponential decay followed by a plateau, then a more rapid fade towards quiescence. The plateau appears to be due to an extra component of optical emission that brightens and then fades over ∼40 days. We show evidence for the origin of this optical 'flare' to be the synchrotron jet during the decaying hard state, and we identify and isolate both disc and jet components in the spectral energy distributions. The optical flare has the same morphology and amplitude as a contemporaneous X-ray rebrightening. This suggests a common origin, but no firm conclusions can be made favouring or disfavouring the jet producing the X-ray flare. The quiescent optical magnitudes are B ≥ 20.6, V ≥ 21.1, R ≥ 19.5, i' ≥ 19.2. From the optical outburst amplitude we estimate a likely orbital period of <22 h. We also present near-infrared (NIR) photometry and polarimetry and rare mid-IR imaging (8-12 μm) when the source is nearing quiescence. The fading jet component, and possibly the companion star, may contribute to the NIR flux. We derive deep mid-IR flux upper limits and NIR linear polarization upper limits. With the inclusion of radio data, we measure an almost flat jet spectral index between radio and optical; F<sub>ν</sub> ν<sup>∼+0.05</sup>. The data favour the jet break to optically thin emission to reside in the IR, but may shift to frequencies as high as the optical or UV during the peak of the flare.</s0> </fC01><fC02 i1="01" i2="3"><s0>001E03</s0></fC02><fC03 i1="01" i2="3" l="FRE"><s0>Jet</s0><s5>26</s5></fC03><fC03 i1="01" i2="3" l="ENG"><s0>Jets</s0><s5>26</s5></fC03><fC03 i1="02" i2="3" l="FRE"><s0>Trou noir</s0><s5>27</s5></fC03><fC03 i1="02" i2="3" l="ENG"><s0>Black holes</s0><s5>27</s5></fC03><fC03 i1="03" i2="X" l="FRE"><s0>Quiescence</s0><s5>28</s5></fC03><fC03 i1="03" i2="X" l="ENG"><s0>Quiescence</s0><s5>28</s5></fC03><fC03 i1="03" i2="X" l="SPA"><s0>Quietud</s0><s5>28</s5></fC03><fC03 i1="04" i2="3" l="FRE"><s0>Courbe lumière</s0><s5>29</s5></fC03><fC03 i1="04" i2="3" l="ENG"><s0>Light curves</s0><s5>29</s5></fC03><fC03 i1="05" i2="X" l="FRE"><s0>Emission optique</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="ENG"><s0>Light emission</s0><s5>30</s5></fC03><fC03 i1="05" i2="X" l="SPA"><s0>Emisión óptica</s0><s5>30</s5></fC03><fC03 i1="06" i2="X" l="FRE"><s0>Sursaut optique</s0><s5>31</s5></fC03><fC03 i1="06" i2="X" l="ENG"><s0>Optical burst</s0><s5>31</s5></fC03><fC03 i1="06" i2="X" l="SPA"><s0>Arrebato óptico</s0><s5>31</s5></fC03><fC03 i1="07" i2="X" l="FRE"><s0>Densité spectrale énergie</s0><s5>32</s5></fC03><fC03 i1="07" i2="X" l="ENG"><s0>Spectral energy distribution</s0><s5>32</s5></fC03><fC03 i1="07" i2="X" l="SPA"><s0>Densidad espectral energía</s0><s5>32</s5></fC03><fC03 i1="08" i2="3" l="FRE"><s0>Morphologie</s0><s5>33</s5></fC03><fC03 i1="08" i2="3" l="ENG"><s0>Morphology</s0><s5>33</s5></fC03><fC03 i1="09" i2="X" l="FRE"><s0>Photométrie IR</s0><s5>34</s5></fC03><fC03 i1="09" i2="X" l="ENG"><s0>Infrared photometry</s0><s5>34</s5></fC03><fC03 i1="09" i2="X" l="SPA"><s0>Fotometría IR</s0><s5>34</s5></fC03><fC03 i1="10" i2="3" l="FRE"><s0>Polarimétrie</s0><s5>35</s5></fC03><fC03 i1="10" i2="3" l="ENG"><s0>Polarimetry</s0><s5>35</s5></fC03><fC03 i1="11" i2="X" l="FRE"><s0>Borne supérieure</s0><s5>36</s5></fC03><fC03 i1="11" i2="X" l="ENG"><s0>Upper bound</s0><s5>36</s5></fC03><fC03 i1="11" i2="X" l="SPA"><s0>Cota superior</s0><s5>36</s5></fC03><fC03 i1="12" i2="3" l="FRE"><s0>Polarisation rectiligne</s0><s5>37</s5></fC03><fC03 i1="12" i2="3" l="ENG"><s0>Linear polarization</s0><s5>37</s5></fC03><fC03 i1="13" i2="3" l="FRE"><s0>Indice spectral</s0><s5>38</s5></fC03><fC03 i1="13" i2="3" l="ENG"><s0>Spectral index</s0><s5>38</s5></fC03><fC03 i1="14" i2="X" l="FRE"><s0>Déplacement fréquence</s0><s5>39</s5></fC03><fC03 i1="14" i2="X" l="ENG"><s0>Frequency shift</s0><s5>39</s5></fC03><fC03 i1="14" i2="X" l="SPA"><s0>Desplazamiento frecuencia</s0><s5>39</s5></fC03><fC03 i1="15" i2="3" l="FRE"><s0>Accrétion</s0><s5>40</s5></fC03><fC03 i1="15" i2="3" l="ENG"><s0>Accretion</s0><s5>40</s5></fC03><fC03 i1="16" i2="3" l="FRE"><s0>Disque accrétion</s0><s5>41</s5></fC03><fC03 i1="16" i2="3" l="ENG"><s0>Accretion disks</s0><s5>41</s5></fC03><fC03 i1="17" i2="3" l="FRE"><s0>Binaire RX</s0><s5>42</s5></fC03><fC03 i1="17" i2="3" l="ENG"><s0>X-ray binary stars</s0><s5>42</s5></fC03><fC03 i1="18" i2="X" l="FRE"><s0>Source RX binaire</s0><s5>43</s5></fC03><fC03 i1="18" i2="X" l="ENG"><s0>Binary X ray source</s0><s5>43</s5></fC03><fC03 i1="18" i2="X" l="SPA"><s0>Fuente RX binaria</s0><s5>43</s5></fC03><fC03 i1="19" i2="3" l="FRE"><s0>Cosmologie</s0><s5>44</s5></fC03><fC03 i1="19" i2="3" l="ENG"><s0>Cosmology</s0><s5>44</s5></fC03><fC03 i1="20" i2="3" l="FRE"><s0>Source RX cosmique</s0><s5>45</s5></fC03><fC03 i1="20" i2="3" l="ENG"><s0>Cosmic x-ray sources</s0><s5>45</s5></fC03><fN21><s1>023</s1></fN21><fN44 i1="01"><s1>OTO</s1></fN44><fN82><s1>OTO</s1></fN82></pA></standard></inist></record>Pour manipuler ce document sous Unix (Dilib)
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|texte= A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752-223
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