Thermal emission from the stellar-mass black hole binary XTE J1118+480 in the low/hard state
dc.contributor.author | Reis, R. C. | en_US |
dc.contributor.author | Miller, J. M. | en_US |
dc.contributor.author | Fabian, A. C. | en_US |
dc.date.accessioned | 2010-04-01T14:55:46Z | |
dc.date.available | 2010-04-01T14:55:46Z | |
dc.date.issued | 2009-05-01 | en_US |
dc.identifier.citation | Reis, R. C.; Miller, J. M.; Fabian, A. C. (2009). "Thermal emission from the stellar-mass black hole binary XTE J1118+480 in the low/hard state." Monthly Notices of the Royal Astronomical Society: Letters 395(1): L52-L56. <http://hdl.handle.net/2027.42/65386> | en_US |
dc.identifier.issn | 1745-3925 | en_US |
dc.identifier.issn | 1745-3933 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/65386 | |
dc.description.abstract | We report on the detection of a thermal disc component from the stellar-mass black hole binary XTE J1118+480 in the canonical low/hard state. The presence of a thermal component with a temperature of approximately 0.21 keV in the Chandra spectra of XTE J1118+480 is found at more than the 14Σ confidence level. Based on this evidence, we argue that the accretion disc in XTE J1118+480 is not truncated far from the central black hole in contrast with previous claims. | en_US |
dc.format.extent | 898749 bytes | |
dc.format.extent | 3110 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.publisher | Blackwell Publishing Ltd | en_US |
dc.rights | Journal compilation © 2009 RAS | en_US |
dc.subject.other | Accretion, Accretion Discs | en_US |
dc.subject.other | Black Hole Physics | en_US |
dc.subject.other | X-rays: Individual: XTE J1118+480 | en_US |
dc.title | Thermal emission from the stellar-mass black hole binary XTE J1118+480 in the low/hard state | 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 | Institute of Astronomy, Madingley Road, Cambridge CB3 0HA | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/65386/1/j.1745-3933.2009.00640.x.pdf | |
dc.identifier.doi | 10.1111/j.1745-3933.2009.00640.x | en_US |
dc.identifier.source | Monthly Notices of the Royal Astronomical Society: Letters | en_US |
dc.identifier.citedreference | Anders E., Grevesse N., 1989, Geochim. Cosmochim. Acta, 53, 197 | en_US |
dc.identifier.citedreference | Arnaud K. A., 1996, in Jacoby G. H., Barnes J., eds, ASP Conf. Ser. Vol. 101, Astronomical Data Analysis Software and Systems V. Astron. Soc. Pac, San Francisco, p. 17 | en_US |
dc.identifier.citedreference | Balucinska-Church M., McCammon D., 1992, ApJ, 400, 699 | en_US |
dc.identifier.citedreference | Brinkman B. C. et al., 2000, in Truemper J. E., Aschenbach B., eds, Proc. SPIE Vol. 4012, X-Ray Optics, Instruments, and Missions III. SPIE, Bellingham, WA, p. 81 | en_US |
dc.identifier.citedreference | Chaty S., Haswell C. A., Malzac J., Hynes R. I., Shrader C. R., Cui W., 2003, MNRAS, 346, 689 | en_US |
dc.identifier.citedreference | Dubus G., Kim R. S. J., Menou K., Szkody P., Bowen D. V., 2001, ApJ, 553, 307 | en_US |
dc.identifier.citedreference | Esin A. A., McClintock J. E., Narayan R., 1997, ApJ, 489, 865 | en_US |
dc.identifier.citedreference | Esin A. A., McClintock J. E., Drake J. J., Garcia M. R., Haswell C. A., Hynes R. I., Muno M. P., 2001, ApJ, 555, 483 | en_US |
dc.identifier.citedreference | Frank J., King A., Raine D., 1992, Accretion Power in Astrophysics, 2nd ed. Cambridge Univ. Press, Cambridge | en_US |
dc.identifier.citedreference | Frontera F. et al., 2001, ApJ, 561, 1006 | en_US |
dc.identifier.citedreference | Fruscione et al., 2006, in Silvia D. R., Doxsey R. E., eds, Proc. SPIE Vol. 6270, Observatory Operations: Strategies, Processes, and Systems. SPIE, Bellingham, WA, p. 62701 | en_US |
dc.identifier.citedreference | Gelino D. M., Balman S., Kiziloglu U., Yilmaz A., Kalemci E., Tomsick J. A., 2006, ApJ, 642, 438 | en_US |
dc.identifier.citedreference | Gierlinski M., Zdziarski A. A., Poutanen J., Coppi P. S., Ebisawa K., Johnson W. N., 1999, MNRAS, 309, 496 | en_US |
dc.identifier.citedreference | Gierlinski M., Done C., Page K., 2008, MNRAS, 388, 753 | en_US |
dc.identifier.citedreference | Hynes R. I., Mauche C. W., Haswell C. A., Shrader C. R., Cui W., Chaty S., 2000, ApJ, 539, L37 | en_US |
dc.identifier.citedreference | Hynes R. I. et al., 2003, MNRAS, 345, 292 | en_US |
dc.identifier.citedreference | Hynes R. I. et al., 2006, ApJ, 651, 401 | en_US |
dc.identifier.citedreference | Kanbach G., Straubmeier C., Spruit H. C., Belloni T., 2001, Nat, 414, 180 | en_US |
dc.identifier.citedreference | King A. R., Ritter H., 1998, MNRAS, 293, L42 | en_US |
dc.identifier.citedreference | Khruzina T. S., Cherepashchuk A. M., Bisikalo D. V., Boyarchuk A. A., Kuznetsov O. A., 2005, Astron. Rep., 49, 79 | en_US |
dc.identifier.citedreference | McClintock J. E., Remillard R. A., 2006, in Lewin W., van der Klis M., eds, Cambridge Astrophys. Ser. 39, Compact Stellar X-ray Sources. Cambridge Univ. Press, Cambridge, p. 157 | en_US |
dc.identifier.citedreference | McClintock J. E. et al., 2001, ApJ, 555, 477 | en_US |
dc.identifier.citedreference | Markoff S., Nowak M. A., 2004, ApJ, 609, 972 | en_US |
dc.identifier.citedreference | Markoff S., Nowak M. A., Wilms J., 2005, ApJ, 635, 1203 | en_US |
dc.identifier.citedreference | Makishima et al., 1986, ApJ, 308, 635 | en_US |
dc.identifier.citedreference | Merloni A., Fabian A. C., 2001, MNRAS, 332, 165 | en_US |
dc.identifier.citedreference | Merloni A., Fabian A. C., 2002, MNRAS, 321, 549 | en_US |
dc.identifier.citedreference | Merloni A., Di Matteo T., Fabian A. C., 2000a, MNRAS, 318, L15 | en_US |
dc.identifier.citedreference | Merloni A., Fabian A. C., Ross R. R., 2000b, MNRAS, 313, 193 | en_US |
dc.identifier.citedreference | Miller J. M., 2007, ARA&A, 45, 441 | en_US |
dc.identifier.citedreference | Miller J. M., Ballantyne D. R., Fabian A. C., Lewin W., H., G., 2002, MNRAS, 335, 865 | en_US |
dc.identifier.citedreference | Miller J. M. et al., 2004, ApJ, 606, L131 | en_US |
dc.identifier.citedreference | Miller J. M., Homan J., Steeghs D., Rupen M., Hunstead R. W., Wijnands R., Charles P. A., Fabian A. C., 2006, ApJ, 653, 525 | en_US |
dc.identifier.citedreference | Miller J. M. et al., 2008, ApJ, 679, L113 | en_US |
dc.identifier.citedreference | Miniutti G., Fabian A. C., Miller J. M., 2004, MNRAS, 351, 466 | en_US |
dc.identifier.citedreference | Mitsuda K. et al., 1984, PASJ, 36, 741 | en_US |
dc.identifier.citedreference | Reis R. C., Fabian A. C., Ross R. R., Miniutti G., Miller J. M., Reynolds C., 2008, MNRAS, 387, 1489 | en_US |
dc.identifier.citedreference | Reis R. C., Fabian A. C., Ross R. R., Miller J. M., 2009, MNRAS, in press ( doi : ) ( arXiv:0902.1745 ) | en_US |
dc.identifier.citedreference | Remillard R. A., McClintock J. E., 2006, ARA&A, 44, 49 | en_US |
dc.identifier.citedreference | Ross R. R., Fabian A. C., 1993, MNRAS, 261, 74 | en_US |
dc.identifier.citedreference | Rykoff E. S., Miller J. M., Steeghs D., Torres M. A. P., 2007, ApJ, 666, 1129 | en_US |
dc.identifier.citedreference | Schlegel D. J., Finkbeiner D. P., Davis M., 1998, ApJ, 500, 525 | en_US |
dc.identifier.citedreference | Shakura N. I., Sunyaev R. A., 1973, A&A, 24, 337 | en_US |
dc.identifier.citedreference | Wagner R. M., Foltz C. B., Shahbaz T., Casares J., Charles P. A., Starfield S. G., Hewett P., 2001, ApJ, 556, 42 | en_US |
dc.identifier.citedreference | Weisskopf M. C., 2004, in Hasinger G., Turner M. J. L., eds, Proc. SPIE Vol. 5488, UV and Gamma-Ray Space Telescope Systems. SPIE, Bellingham, WA, p. 25 | en_US |
dc.identifier.citedreference | Yamaoka K., Ueda Y., Dotani T., Durouchoux P., Rodriguez J., 2000, IAU Circ. 7427 | en_US |
dc.identifier.citedreference | Zurita C. et al., 2002, MNRAS, 333, 791 | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
Files in this item
Remediation of Harmful Language
The University of Michigan Library aims to describe library materials in a way that respects the people and communities who create, use, and are represented in our collections. Report harmful or offensive language in catalog records, finding aids, or elsewhere in our collections anonymously through our metadata feedback form. More information at Remediation of Harmful Language.
Accessibility
If you are unable to use this file in its current format, please select the Contact Us link and we can modify it to make it more accessible to you.