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The eccentric accretion disc of the black hole A0620-00

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Neilsen, J., Steeghs, D. (Danny), 1972- and Vrtilek, Saeqa Dil. (2008) The eccentric accretion disc of the black hole A0620-00. Monthly Notices of the Royal Astronomical Society, Vol.384 (No.3). pp. 849-862. ISSN 0035-8711

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Official URL: http://dx.doi.org/10.1111/j.1365-2966.2007.12599.x

Abstract

We present spectroscopic observations of the quiescent black hole binary A0620-00 with the 6.5-m Magellan Clay telescope at Las Campanas Observatory. We measure absorption-line radial velocities of the secondary and make the most precise determination to date (K-2 = 435.4 +/- 0.5 km s(-1)). By fitting the rotational broadening of the secondary, we refine the mass ratio to q = 0.060 +/- 0.004; these results, combined with the orbital period, imply a minimum mass for the compact object of 3.10 +/- 0.04 M-circle dot. Although quiescence implies little accretion activity, we find that the disc contributes 56 +/- 7 per cent of the light in B and V, and is subject to significant flickering. Doppler maps of the Balmer lines reveal bright emission from the gas stream-disc impact point and unusual crescent-shaped features. We also find that the disc centre of symmetry does not coincide with the predicted black hole velocity. By comparison with smoothed particle hydrodynamics (SPH) simulations, we identify this source with an eccentric disc. With high signal-to-noise ratio (S/N), we pursue modulation tomography of H alpha and find that the aforementioned bright regions are strongly modulated at the orbital period. We interpret this modulation in the context of disc precession, and discuss cases for the accretion disc evolution.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Black holes (Astronomy), Double stars, Accretion (Astrophysics)
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Wiley-Blackwell Publishing, Inc
ISSN: 0035-8711
Date: 1 March 2008
Volume: Vol.384
Number: No.3
Number of Pages: 14
Page Range: pp. 849-862
Identification Number: 10.1111/j.1365-2966.2007.12599.x
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: National Science Foundation (U.S.) (NSF), Harvard University. Graduate School of Arts and Sciences, Smithsonian Astrophysical Observatory
Grant number: AST- 0507637 (NSF)
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References: Elvis M., Griffiths C.G., Turner M.J.L., Page C., 1975, IAU Circ, 2184 Frank J., King A., Raine D., 2002, Accretion Power in Astrophysics. Cambridge University Press, Cambridge, UK Foulkes S.B., Haswell C.A., Murray J.R., Rolfe D.J., 2004, MNRAS, 349, 1179 Friedman J.L., Ipser J.R., 1987, ApJ, 314, 594 Froning C.S., Robinson E.L., 2001, AJ, 121, 2212 Froning C.S., Robinson E.L., Bitner M.A., 2007, ApJ, in press Gelino D.M., Harrison T.E., Orosz J.A., 2001, AJ, 122, 2668 Johnston H.M., Kulkarni S.R., Oke J.B., 1989, ApJ, 345, 492 Leibowitz E.M., Hemar S., Orio M., 1998, MNRAS, 300, 463L Malaroda S., Levato H., Galliani S., 2001, VizieR On-line Data Catalog: III/216. Marsh T.R., 2001, in Boffin H.M.J., Steeghs D., Cuypers J., eds, LNP Vol. 573, Astrotomography: Indirect Imaging Methods in Observational Astronomy. Springer-Verlag, Berlin, p. 1 Marsh T.R., Horne K., Schlegel E.M., Honeycutt R.K., Kaitchuck R.H. 1990, ApJ, 364, 637 Marsh T.R., Robinson E.L., Wood J.H., 1994, MNRAS, 266, 137 (MRW94) McClintock J.E., Remillard R.A., 1986, ApJ, 308, 110 (MR86) McClintock J.E., Horne K., Remillard R.A., 1995, ApJ, 442, 358 Paczynski B., 1971, ARA&A, 9, 183 Shahbaz T., Naylor T., Charles P.A., 1994, MNRAS, 268, 756 Shahbaz T., Bandyopadhyay R.M., Charles P.A., 1999, A&A, 346, 82 Shahbaz T., Hynes R.I., Charles P.A., Zurita C., Casares J., Haswell C.A., Araujo-Betancor S., Powell C., 2004, MNRAS, 354, 31 (S04) Smith A.J., Haswell C.A., Murray J.R., Truss M.R., Foulkes S.B., 2007, MNRAS, 378, 785 Steeghs D., 2003, MNRAS, 344, 448 Steeghs D., Casares J., 2002, ApJ, 568, 273 Sterne T.E., 1941, PNAS, 27, 168 Wade R.A., Rucinski S.M., 1985, A&SS, 60, 471 Whitehurst R., King A., 1991, MNRAS, 249, 25
URI: http://wrap.warwick.ac.uk/id/eprint/30454

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