The black hole candidate XTE J1752−223 towards and in quiescence: optical and simultaneous X‐ray–radio observations
dc.contributor.author | Ratti, E. M. | en_US |
dc.contributor.author | Jonker, P. G. | en_US |
dc.contributor.author | Miller‐jones, J. C. A. | en_US |
dc.contributor.author | Torres, M. A. P. | en_US |
dc.contributor.author | Homan, J. | en_US |
dc.contributor.author | Markoff, S. | en_US |
dc.contributor.author | Tomsick, J. A. | en_US |
dc.contributor.author | Kaaret, P. | en_US |
dc.contributor.author | Wijnands, R. | en_US |
dc.contributor.author | Gallo, E. | en_US |
dc.contributor.author | Özel, F. | en_US |
dc.contributor.author | Steeghs, D. T. H. | en_US |
dc.contributor.author | Fender, R. P. | en_US |
dc.date.accessioned | 2012-07-12T17:25:50Z | |
dc.date.available | 2013-09-03T15:38:27Z | en_US |
dc.date.issued | 2012-07-01 | en_US |
dc.identifier.citation | Ratti, E. M.; Jonker, P. G.; Miller‐jones, J. C. A. ; Torres, M. A. P.; Homan, J.; Markoff, S.; Tomsick, J. A.; Kaaret, P.; Wijnands, R.; Gallo, E.; Özel, F. ; Steeghs, D. T. H.; Fender, R. P. (2012). "The black hole candidate XTE J1752â 223 towards and in quiescence: optical and simultaneous Xâ rayâ radio observations." Monthly Notices of the Royal Astronomical Society 423(3). <http://hdl.handle.net/2027.42/92116> | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.issn | 1365-2966 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/92116 | |
dc.description.abstract | We present optical, X‐ray and radio observations of the black hole transient (BHT) XTE J1752−223 towards and in quiescence. Optical photometry shows that the quiescent magnitude of XTE J1752−223 is fainter than 24.4 mag in the i ′ band. A comparison with measurements of the source during its 2009–2010 outburst shows that the outburst amplitude is more than 8 mag in the i ′ band. Known X‐ray properties of the source combined with the faintness of the quiescence optical counterpart and the large outburst optical amplitude point towards a short orbital‐period system ( P orb ≲ 6.8 h) with an M type (or later) mass donor, at a distance of 3.5 ≲ d ≲ 8 kpc. Simultaneous X‐ray and radio data were collected with Chandra and the Expanded Very Large Array (EVLA), allowing constraints to be placed on the quiescent X‐ray and radio flux of XTE J1752−223. Furthermore, using data covering the final stage of the outburst decay, we investigated the low‐luminosity end of the X‐ray–radio correlation for this source and compared it with other BHTs. We found that XTE J1752−223 adds to the number of outliers with respect to the ‘standard’ X‐ray–radio luminosity relation. Furthermore, XTE J1752−223 is the second source, after the BHT H1743−322, that shows a transition from the region of the outliers towards the ‘standard’ correlation at low luminosity. Finally, we report on a faint, variable X‐ray source we discovered with Chandra at an angular distance of ∼2.9 arcsec to XTE J1752−223 and at a position angle consistent with that of the radio jets previously observed from the BHT. We discuss the possibility that we detected X‐ray emission associated with a jet from XTE J1752−223. | en_US |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.publisher | Wiley Periodicals, Inc. | en_US |
dc.subject.other | Binaries: General | en_US |
dc.subject.other | Stars: Individual: XTE J1752−223 | en_US |
dc.subject.other | X‐Rays: Binaries | en_US |
dc.subject.other | Accretion, Accretion Discs | en_US |
dc.title | The black hole candidate XTE J1752−223 towards and in quiescence: optical and simultaneous X‐ray–radio observations | 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 St, Ann Arbor, MI 48109, USA | en_US |
dc.contributor.affiliationother | Department of Astrophysics, IMAPP, Radboud University Nijmegen, Heyendaalseweg 135, 6525 AJ, Nijmegen, the Netherlands | 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 | School of Physics and Astronomy, University of Southampton, Highfield, Southampton SO17 1BJ | en_US |
dc.contributor.affiliationother | Department of Physics, University of Warwick, Coventry CV4 7AL | en_US |
dc.contributor.affiliationother | Department of Astronomy, University of Arizona, 933 N. Cherry Ave., Tucson, AZ 85721, USA | en_US |
dc.contributor.affiliationother | Department of Physics and Astronomy, University of Iowa, Iowa City, IA 52242, USA | en_US |
dc.contributor.affiliationother | Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, CA 94720‐7450, 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 | MIT Kavli Institute for Astrophysics and Space Research, 70 Vassar Street, Cambridge, MA 02139, USA | en_US |
dc.contributor.affiliationother | International Centre for Radio Astronomy Research – Curtin University, GPO Box U1987, Perth, WA 6845, Australia | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/92116/1/j.1365-2966.2012.21071.x.pdf | |
dc.identifier.doi | 10.1111/j.1365-2966.2012.21071.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society | en_US |
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