A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752−223 ★
dc.contributor.author | Russell, D. M. | en_US |
dc.contributor.author | Curran, P. A. | en_US |
dc.contributor.author | Muñoz‐darias, T. | en_US |
dc.contributor.author | Lewis, F. | en_US |
dc.contributor.author | Motta, S. | en_US |
dc.contributor.author | Stiele, H. | en_US |
dc.contributor.author | Belloni, Tomaso | en_US |
dc.contributor.author | Miller‐jones, J. C. A. | en_US |
dc.contributor.author | Jonker, P. G. | en_US |
dc.contributor.author | O’brien, K. | en_US |
dc.contributor.author | Homan, Jeroen | en_US |
dc.contributor.author | Casella, P. | en_US |
dc.contributor.author | Gandhi, P. | en_US |
dc.contributor.author | Soleri, P. | en_US |
dc.contributor.author | Markoff, Sera | en_US |
dc.contributor.author | Maitra, Dipankar | en_US |
dc.contributor.author | Gallo, E. | en_US |
dc.contributor.author | Cadolle Bel, M. | en_US |
dc.date.accessioned | 2012-01-05T22:06:03Z | |
dc.date.available | 2013-03-04T15:29:54Z | en_US |
dc.date.issued | 2012-01-11 | en_US |
dc.identifier.citation | Russell, D. M.; Curran, P. A.; Muñoz‐darias, T. ; Lewis, F.; Motta, S.; Stiele, H.; Belloni, T.; Miller‐jones, J. C. A. ; Jonker, P. G.; O’brien, K. ; Homan, J.; Casella, P.; Gandhi, P.; Soleri, P.; Markoff, S.; Maitra, D.; Gallo, E.; Cadolle Bel, M. (2012). "A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752â 223 â ." Monthly Notices of the Royal Astronomical Society 419(2). <http://hdl.handle.net/2027.42/89507> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/89507 | |
dc.description.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 m) 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 ν ∝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. | en_US |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Accretion, Accretion Discs | en_US |
dc.subject.other | Black Hole Physics | en_US |
dc.subject.other | ISM: Jets and Outflows | en_US |
dc.subject.other | X‐Rays: Binaries | en_US |
dc.title | A late jet rebrightening revealed from multiwavelength monitoring of the black hole candidate XTE J1752−223 ★ | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Astronomy | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Department of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | Astronomical Institute ‘Anton Pannekoek’, University of Amsterdam, PO Box 94249, 1090 GE Amsterdam, the Netherlands | en_US |
dc.contributor.affiliationother | Laboratoire AIM, CEA/IRFU‐Université Paris Diderot‐CNRS/INSU, CEA DSM/IRFU/SAp, Centre de Saclay, F‐91191 Gif‐sur‐Yvette, France | en_US |
dc.contributor.affiliationother | INAF–Osservatorio Astronomico di Brera, Via E. Bianchi 46, I‐23807 Merate (LC), Italy | en_US |
dc.contributor.affiliationother | Faulkes Telescope Project, University of Glamorgan, Pontypridd CF37 1DL | en_US |
dc.contributor.affiliationother | Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes MK7 6AA | en_US |
dc.contributor.affiliationother | International Centre for Radio Astronomy Research, Curtin University, GPO Box U1987, Perth, WA 6845, Australia | en_US |
dc.contributor.affiliationother | SRON, Netherlands Institute for Space Research, Sorbonnelaan 2, 3584 CA, Utrecht, the Netherlands | en_US |
dc.contributor.affiliationother | Harvard–Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA | en_US |
dc.contributor.affiliationother | Department of Astrophysics, IMAPP, Radboud University Nijmegen, PO Box 9010, NL‐6500 GL Nijmegen, the Netherlands | en_US |
dc.contributor.affiliationother | Department of Physics, University of California, Santa Barbara, CA 93106‐9530, USA | en_US |
dc.contributor.affiliationother | MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street, Cambridge, MA 02139, USA | en_US |
dc.contributor.affiliationother | School of Physics and Astronomy, University of Southampton, Southampton, Hampshire SO17 1BJ | en_US |
dc.contributor.affiliationother | ISAS, Japan Aerospace Exploration Agency, 3‐1‐1 Yoshinodai, chuo‐ku, Sagamihara, Kanagawa 229‐8510, Japan | en_US |
dc.contributor.affiliationother | Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen, the Netherlands | en_US |
dc.contributor.affiliationother | ESAC, ISOC, Villanueva de la Cañada, Madrid P. O. Box 78, E‐28691, Spain | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/89507/1/j.1365-2966.2011.19839.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2011.19839.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
dc.identifier.citedreference | Barrena R., Acosta‐Pulido J. A., Manchado A., 2008, in Kaufer A., Kerber F., eds, ESO Astrophysics Symposia, Proc. ‘The 2007 ESO Instrument Calibration Workshop’. Springer‐Verlag, Berlin, p. 511 | en_US |
dc.identifier.citedreference | Belloni T. M., 2010, in Belloni T., ed., Lecture Notes in Physics Vol. 794, The Jet Paradigm – From Microquasars to Quasars. Springer‐Verlag, Berlin, p. 53 | en_US |
dc.identifier.citedreference | Belloni T., Hasinger G., 1990, A&A, 230, 103 | en_US |
dc.identifier.citedreference | Björnsson C. I., Blumenthal G. R., 1982, ApJ, 259, 805 | en_US |
dc.identifier.citedreference | Breeveld A. A. et al., 2010, MNRAS, 406, 1687 | en_US |
dc.identifier.citedreference | Brocksopp C., Miller‐Jones J. C. A., Fender R. P., Stappers B. W., 2007, MNRAS, 378, 1111 | en_US |
dc.identifier.citedreference | Brocksopp C., Corbel S., Tzioumis T., Fender R., 2009, Astron. Telegram, 2278 | en_US |
dc.identifier.citedreference | Buxton M. M., Bailyn C. D., 2004, ApJ, 615, 880 | en_US |
dc.identifier.citedreference | Callanan P. J. et al., 1995, ApJ, 441, 786 | en_US |
dc.identifier.citedreference | Calvelo D. E. et al., 2010, MNRAS, 409, 839 | en_US |
dc.identifier.citedreference | Cardelli J. A., Clayton G. C., Mathis J. S., 1989, ApJ, 345, 245 | en_US |
dc.identifier.citedreference | Casella P. et al., 2010, MNRAS, 404, L21 | en_US |
dc.identifier.citedreference | Chaty S., Dubus G., Raichoor A., 2011, A&A, 529, 3 | en_US |
dc.identifier.citedreference | Chen W., Shrader C. R., Livio M., 1997, ApJ, 491, 312 | en_US |
dc.identifier.citedreference | Chiang C. Y., Done C., Still M., Godet O., 2010, MNRAS, 403, 1102 | en_US |
dc.identifier.citedreference | Corbel S., Fender R. P., 2002, ApJ, 573, L35 | en_US |
dc.identifier.citedreference | Corbel S., Fender R. P., Tzioumis A. K., Nowak M., McIntyre V., Durouchoux P., Sood R., 2000, A&A, 359, 251 | en_US |
dc.identifier.citedreference | Corbel S., Nowak M. A., Fender R. P., Tzioumis A. K., Markoff S., 2003, A&A, 400, 1007 | en_US |
dc.identifier.citedreference | Coriat M., Corbel S., Buxton M. M., Bailyn C. D., Tomsick J. A., Körding E., Kalemci E., 2009, MNRAS, 400, 123 | en_US |
dc.identifier.citedreference | Coriat M. et al., 2011, MNRAS, 414, 677 | en_US |
dc.identifier.citedreference | Corral‐Santana J. M., Casares J. P. Rodríguez‐Gil P., 2010, Astron. Telegram, 2805 | en_US |
dc.identifier.citedreference | Cox A. N., 2000, Allen’s Astrophysical Quantities, 4th edn. Am. Inst. Phys., New York | en_US |
dc.identifier.citedreference | Curran P. A., Maccarone T. J., Casella P., Evans P. A., Landsman W., Krimm H. A., Brocksopp C., Still M., 2011, MNRAS, 410, 541 (C11) | en_US |
dc.identifier.citedreference | Dunn R. J. H., Fender R. P., Körding E. G., Belloni T., Cabanac C., 2010, MNRAS, 403, 61 | en_US |
dc.identifier.citedreference | Eikenberry S. S., Matthews K., Morgan E. H., Remillard R. A., Nelson R. W., 1998, ApJ, 494, L61 | en_US |
dc.identifier.citedreference | Erben T. et al., 2005, Astron. Nachr., 326, 432 | en_US |
dc.identifier.citedreference | Evans W. D., Belian R. D., Conner J. P., 1970, ApJ, 159, L57 | en_US |
dc.identifier.citedreference | Falcke H., Biermann P. L., 1995, A&A, 293, 665 | en_US |
dc.identifier.citedreference | Fender R. P., 2001, MNRAS, 322, 31 | en_US |
dc.identifier.citedreference | Fender R. P., Rayner D., McCormick D. G., Muxlow T. W. B., Pooley G. G., Sault R. J., Spencer R. E., 2002, MNRAS, 336, 39 | en_US |
dc.identifier.citedreference | Fender R. P., Belloni T. M., Gallo E., 2004, MNRAS, 355, 1105 | en_US |
dc.identifier.citedreference | Fender R. P., Homan J., Belloni T. M., 2009, MNRAS, 396, 1370 | en_US |
dc.identifier.citedreference | Frank J., King A., Raine D. J., 2002, Accretion Power in Astrophysics, 3rd edn. Cambridge Univ. Press, Cambridge | en_US |
dc.identifier.citedreference | Gallo E., Fender R. P., Pooley G. G., 2003, MNRAS, 344, 60 | en_US |
dc.identifier.citedreference | Gallo E. et al., 2006, MNRAS, 370, 1351 | en_US |
dc.identifier.citedreference | Gallo E., Migliari S., Markoff S., Tomsick J. A., Bailyn C. D., Berta S., Fender R., Miller‐Jones J. C. A., 2007, ApJ, 670, 600 | en_US |
dc.identifier.citedreference | Gandhi P. et al., 2010, MNRAS, 407, 2166 | en_US |
dc.identifier.citedreference | Gandhi P. et al., 2011, ApJ, 740, L13 | en_US |
dc.identifier.citedreference | Gierliński M., Done C., Page K., 2009, MNRAS, 392, 1106 | en_US |
dc.identifier.citedreference | Hannikainen D. C., Hunstead R. W., Campbell‐Wilson D., Sood R. K., 1998, A&A, 337, 460 | en_US |
dc.identifier.citedreference | Heinz S., Sunyaev R. A., 2003, MNRAS, 343, L59 | en_US |
dc.identifier.citedreference | Homan J., Buxton M., Markoff S., Bailyn C. D., Nespoli E., Belloni T., 2005, ApJ, 624, 295 | en_US |
dc.identifier.citedreference | Hynes R. I., 2005, ApJ, 623, 1026 | en_US |
dc.identifier.citedreference | Jain R. K., Bailyn C. D., Orosz J. A., McClintock J. E., Remillard R. A., 2001, ApJ, 554, L181 | en_US |
dc.identifier.citedreference | Jordi K., Grebel E. K., Ammon K., 2006, A&A, 460, 339 | en_US |
dc.identifier.citedreference | Kalemci E., Tomsick J. A., Rothschild R. E., Pottschmidt K., Corbel S., Kaaret P., 2006, ApJ, 639, 340 | en_US |
dc.identifier.citedreference | Kalemci E., Chun Y. Y., Dincer T., Buxton M., Tomsick J. A., Corbel S., Kaaret P., 2011, in Romero G., Sunyaev R., Bellon T., eds, IAU Symp. 275. Jets at All Scales. Cambridge Univ. Press, Cambridge, p. 299 | en_US |
dc.identifier.citedreference | King A. R., 1993, MNRAS, 260, L5 | en_US |
dc.identifier.citedreference | Körding E., Fender R. P., Migliari S., 2006, MNRAS, 369, 1451 | en_US |
dc.identifier.citedreference | Kuulkers E., 1998, New Astron. Rev., 42, 1 | en_US |
dc.identifier.citedreference | Lasota J. P., 2008, New Astron. Rev., 51, 752 | en_US |
dc.identifier.citedreference | Laurent P., Rodriguez J., Wilms J., Cadolle Bel M., Pottschmidt K., Grinberg V., 2011, Sci, 332, 438 | en_US |
dc.identifier.citedreference | Lewis F., Russell D. M., Fender R. P., Roche P., Clark S. J., 2008, in Proc. VII Microquasar Workshop: Microquasars and Beyond, Proceedings of Science. SISSA, Trieste, PoS(MQW7)069 | en_US |
dc.identifier.citedreference | Lewis F. et al., 2010, A&A, 517, A72 | en_US |
dc.identifier.citedreference | Maitra D., Bailyn C. D., 2008, ApJ, 688, 537 | en_US |
dc.identifier.citedreference | Markoff S., Falcke H., Fender R., 2001, A&A, 372, L25 | en_US |
dc.identifier.citedreference | Markoff S., Nowak M., Corbel S., Fender R., Falcke H., 2003, A&A, 397, 645 | en_US |
dc.identifier.citedreference | Markoff S., Nowak M. A., Wilms J., 2005, ApJ, 635, 1203 | en_US |
dc.identifier.citedreference | Markwardt C. B. et al., 2009, Astron. Telegram, 2258 | en_US |
dc.identifier.citedreference | Migliari S., Fender R. P., 2006, MNRAS, 366, 79 | en_US |
dc.identifier.citedreference | Migliari S., Tomsick J. A., Maccarone T. J., Gallo E., Fender R. P., Nelemans G., Russell D. M., 2006, ApJ, 643, L41 | en_US |
dc.identifier.citedreference | Migliari S. et al., 2007, ApJ, 670, 610 | en_US |
dc.identifier.citedreference | Migliari S. et al., 2010, ApJ, 710, 117 | en_US |
dc.identifier.citedreference | Miller‐Jones J. C. A., Jonker P. G., Ratti E., Torres M. A. P., Brocksopp C., Yang J., Morrell N., 2011, MNRAS, 415, 306 | en_US |
dc.identifier.citedreference | Motch C., Ilovaisky S. A., Chevalier C., Angebault P., 1985, Space Sci. Rev., 40, 219 | en_US |
dc.identifier.citedreference | Motta S., Muñoz‐Darias T., Belloni T., 2010, MNRAS, 408, 1796 | en_US |
dc.identifier.citedreference | Muñoz‐Darias T., Casares J., Martínez‐Pais I. G., 2008, MNRAS, 385, 2205 | en_US |
dc.identifier.citedreference | Muñoz‐Darias T., Motta S., Pawar D., Belloni T. M., Campana S., Bhattacharya D., 2010, MNRAS, 404, L94 | en_US |
dc.identifier.citedreference | Nakahira S. et al., 2010, PASJ, 62, L27 | en_US |
dc.identifier.citedreference | Pe’er A., Casella P., 2009, ApJ, 699, 1919 | en_US |
dc.identifier.citedreference | Poole T. S. et al., 2008, MNRAS, 383, 627 | en_US |
dc.identifier.citedreference | Predehl P., Schmitt J. H. M. M., 1995, A&A, 293, 889 | en_US |
dc.identifier.citedreference | Rahoui F., Lee J. C., Heinz S., Hines D. C., Pottschmidt K., Wilms J., Grinberg V., 2011, ApJ, 736, 63 | en_US |
dc.identifier.citedreference | Roming P. W. A. et al., 2005, Space Sci. Rev., 120, 95 | en_US |
dc.identifier.citedreference | Ruelas‐Mayorga R. A., 1991, Rev. Mex. Astron. Astrofis. 22, 27 | en_US |
dc.identifier.citedreference | Russell D. M., Fender R. P., 2008, MNRAS, 387, 713 | en_US |
dc.identifier.citedreference | Russell D. M., Fender R. P., Hynes R. I., Brocksopp C., Homan J., Jonker P. G., Buxton M. M., 2006, MNRAS, 371, 1334 | en_US |
dc.identifier.citedreference | Russell D. M., Maitra D., Dunn R. J. H., Markoff S., 2010a, MNRAS, 405, 1759 | en_US |
dc.identifier.citedreference | Russell D. M., Muñoz‐Darias T., Lewis F., Soleri P., 2010b, Astron. Telegram, 2775 | en_US |
dc.identifier.citedreference | Russell D. M., Casella P., Fender R., Soleri P., Pretorius M. L., Lewis F., van der Klis M., 2011a, in Proc. ‘High Time Resolution Astrophysics IV – The Era of Extremely Large Telescopes – HTRA IV’, Proceedings of Science. SISSA, Trieste, PoS (MQW7)002 | en_US |
dc.identifier.citedreference | Russell D. M., Maitra D., Dunn R. J. H., Fender R. P., 2011b, MNRAS, 416, 2311 | en_US |
dc.identifier.citedreference | Rybicki G. B., Lightman A. P., 1979, Radiative Processes in Astrophysics. Wiley, New York | en_US |
dc.identifier.citedreference | Shahbaz T., Kuulkers E., 1998, MNRAS, 295, L1 | en_US |
dc.identifier.citedreference | Shahbaz T., Fender R. P., Watson C. A., O’Brien K., 2008, ApJ, 672, 510 | en_US |
dc.identifier.citedreference | Shaposhnikov N., Markwardt C., Swank J., Krimm H., 2010, ApJ, 723, 1817 | en_US |
dc.identifier.citedreference | Soleri P., Fender R., 2011, MNRAS, 413, 2269 | en_US |
dc.identifier.citedreference | Stiele H., Muñoz‐Darias T., Motta S., Belloni T., 2011, Proc. 25th Texas Symposium on Relativistic Astrophysics – TEXAS 2010. SISSA, Trieste, PoS (Texas2010)032 | en_US |
dc.identifier.citedreference | Tananbaum H., Gursky H., Kellogg E., Giacconi R., Jones C., 1972, ApJ, 177, L5 | en_US |
dc.identifier.citedreference | Torres M. A. P., Jonker P. G., Steeghs D., Yan H., Huang J., Soderberg A. M., 2009a, Astron. Telegram, 2263 | en_US |
dc.identifier.citedreference | Torres M. A. P., Steeghs D., Jonker P. G., Thompson I., Soderberg A. M., 2009b, Astron. Telegram, 2268 | en_US |
dc.identifier.citedreference | van Paradijs J., McClintock J. E., 1994, A&A, 290, 133 | en_US |
dc.identifier.citedreference | Yang J., Brocksopp C., Corbel S., Paragi Z., Tzioumis T., Fender R. P., 2010, MNRAS, 409, L64 | en_US |
dc.identifier.citedreference | Yang J., Paragi Z., Corbel S., Gurvits L. I., Campbell R. M., Brocksopp C., 2011, MNRAS, preprint (arXiv:1108.3492) | en_US |
dc.identifier.citedreference | Zurita Heras J. A., Chaty S., Cadolle Bel M., Prat L., 2011, MNRAS, 413, 235 | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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