Radio monitoring of the hard state jets in the 2011 outburst of MAXI J1836-194

Autor: A. Moin, Gregory R. Sivakoff, Ronald A. Remillard, Anastasios Tzioumis, M. A. P. Torres, Sera Markoff, Craig L. Sarazin, Stephane Corbel, Peter G. Jonker, T. Slaven-Blair, Michael P. Rupen, Valeriu Tudose, Alexandra J. Tetarenko, Dipankar Maitra, Thomas D. Russell, P. A. Curran, D. M. Russell, Mickael Coriat, James Miller-Jones, Diego Altamirano, Roberto Soria, Sebastian Heinz, T. M. Belloni, Rob Fender, Matthew J. Middleton, Elmar Körding, Simone Migliari, Hans A. Krimm
Přispěvatelé: Curtin University [Perth], Planning and Transport Research Centre (PATREC), Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), School of Physics and Astronomy [Southampton], University of Southampton, Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), New York University [Abu Dhabi], NYU System (NYU), Department of Physics [Edmonton], University of Alberta, INAF - Osservatorio Astronomico di Brera (OAB), Istituto Nazionale di Astrofisica (INAF), Université Grenoble Alpes - UFR Médecine (UGA UFRM), Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), University of Wisconsin-Madison, SRON Netherlands Institute for Space Research (SRON), NASA Goddard Space Flight Center (GSFC), Radboud University [Nijmegen], Wheaton College [Norton], University of Amsterdam [Amsterdam] (UvA), CRUK Medical Oncology Unit, The Churchill Hospital, University of Barcelona, MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology (MIT), NRC Herzberg Astronomy and Astrophysics, Conseil National de Recherches Canada (CNRC), National Radio Astronomy Observatory [Socorro] (NRAO), National Radio Astronomy Observatory (NRAO), Laboratoire Sciences Analytiques, Bioanalytiques, et Miniaturisation (LSABM), Chimie-Biologie-Innovation (UMR 8231) (CBI), Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS)-Ecole Superieure de Physique et de Chimie Industrielles de la Ville de Paris (ESPCI Paris), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut de Chimie du CNRS (INC)-Centre National de la Recherche Scientifique (CNRS), Universidad Nacional de Entre Ríos [Argentine] (UNER), Institute of Space Science [Bucharest-Măgurele] (ISS), CSIRO Astronomy and Space Science, Commonwealth Scientific and Industrial Research Organisation [Canberra] (CSIRO), Australian Research Council DP 120102393 Spanish Ministerio de Ciencia e Innovacion AYA2013-47447-C03-1-P, ANR-12-BS05-0009,CHAOS,Caractérisation des processus d'accretion-ejection dans les systèmes binaires compacts(2012), ANR-11-IDEX-0005,USPC,Université Sorbonne Paris Cité(2011), API (FNWI), Astrophysique Interprétation Modélisation (AIM (UMR_7158 / UMR_E_9005 / UM_112)), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Radboud university [Nijmegen], Université d'Orléans (UO)-Observatoire des Sciences de l'Univers en région Centre (OSUC), PSL Research University (PSL)-PSL Research University (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-Centre National de la Recherche Scientifique (CNRS), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Grenoble Alpes (UGA), National Optical Astronomy Observatory (NOAO), National Optical Astronomy Observatory, ESPCI ParisTech-Centre National de la Recherche Scientifique (CNRS), ANR-11-IDEX-0005-02/10-LABX-0023,UnivEarthS,Earth - Planets - Universe: observation, modeling, transfer(2011), Department of Astronomy, Faculty of Science
Jazyk: angličtina
Rok vydání: 2015
Předmět:
stars: individual: MAXI J1836−194
Astronomy
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Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2015, 450 (2), pp.1745-1759. ⟨10.1093/mnras/stv723⟩
Monthly Notices of the Royal Astronomical Society, 450(2), 1745-1759. Oxford University Press
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 450 (2), pp.1745-1759. ⟨10.1093/mnras/stv723⟩
Monthly Notices of the Royal Astronomical Society, 450, 2, pp. 1745-1759
Monthly Notices of the Royal Astronomical Society, 450, 1745-1759
ISSN: 0035-8711
1365-2966
DOI: 10.1093/mnras/stv723⟩
Popis: MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its `failed' outburst, in which the source did not complete a full set of state changes, only transitioning as far as the hard intermediate state. Observations with the Karl G. Jansky Very Large Array (VLA) and Australia Telescope Compact Array (ATCA) show that the jet properties changed significantly during the outburst. The VLA observations detected linearly polarised emission at a level of ~1% early in the outburst, increasing to ~3% as the outburst peaked. High-resolution images with the Very Long Baseline Array (VLBA) show a ~15 mas jet along the position angle $-21 \pm 2^\circ$, in agreement with the electric vector position angle found from our polarisation results ($-21 \pm 4^\circ$), implying that the magnetic field is perpendicular to the jet. Astrometric observations suggest that the system required an asymmetric natal kick to explain its observed space velocity. Comparing quasi-simultaneous X-ray monitoring with the 5 GHz VLA observations from the 2011 outburst shows an unusually steep hard-state radio/X-ray correlation of $L_{\rm R} \propto L_{\rm X}^{1.8\pm0.2}$, where $L_{\rm R}$ and $L_{\rm X}$ denote the radio and X-ray luminosities, respectively. With ATCA and Swift monitoring of the source during a period of re-brightening in 2012, we show that the system lay on the same steep correlation. Due to the low inclination of this system, we then investigate the possibility that the observed correlation may have been steepened by variable Doppler boosting.
18 pages, 4 tables, 10 figures. Accepted for publication in MNRAS
Databáze: OpenAIRE
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