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  • 1
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    GRS 1739-278 Observed at Very Low Luminosity with XMM-Newton and NuSTAR (2016)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS1739278 during a very faint low hard state at 0.02% of the Eddington luminosity (for a distance of 8.5 kpc and a mass of 10 solar mass). The broadband X-ray spectrum between 0.5 and 60 keV can be well-described by a power-law continuum with an exponential cutoff. The continuum is unusually hard for such a low luminosity, with a photon index of =1.39+/-0.04. We find evidence for an additional reflection component from an optically thick accretion disk at the 98% likelihood level. The reflection fraction is low, with R(sub refl) = 0.043(exp + 0.033)(sub - 0.023). In combination with measurements of the spin and inclination parameters made with NuSTAR during a brighter hard state by Miller et al., we seek to constrain the accretion disk geometry. Depending on the assumed emissivity profile of the accretion disk, we find a truncation radius of 15-35 R(sub g) (5-12 R(sub ISCO)) at the 90% confidence limit. These values depend strongly on the assumptions and we discuss possible systematic uncertainties.
    Keywords: Astrophysics
    Type: GSFC-E-DAA-TN60680 , The Astrophysical Journal (ISSN 0004-637X) (e-ISSN 1538-4357); 832; 2; 115
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  • 2
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    Space Telescope and Optical Reverberation Mapping Project. VI. Reverberating Disk Models for NGS 5548 (2017)
    In:  Other Sources
    Details
    Publication Date: 2019-07-13
    Description: We conduct a multi-wavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investigate the temperature structure of its accretion disk. The 19 overlapping continuum light curves (1158 Angstrom to 9157 Angstrom) combine simultaneous Hubble Space Telescope, Swift, and ground-based observations over a 180 day period from 2014 January to July. Light-curve variability is interpreted as the reverberation response of the accretion disk to irradiation by a central time-varying point source. Our model yields the disk inclination i = 36deg +/- 10deg, temperature T(sub 1) = (44+/-6) times 10 (exp 3)K at 1 light day from the black hole, and a temperature radius slope (T proportional to r (exp -alpha)) of alpha = 0.99 +/- 0.03. We also infer the driving light curve and find that it correlates poorly with both the hard and soft X-ray light curves, suggesting that the X-rays alone may not drive the ultraviolet and optical variability over the observing period. We also decompose the light curves into bright, faint, and mean accretion-disk spectra. These spectra lie below that expected for a standard blackbody accretion disk accreting at L/L(sub Edd) = 0.1.
    Keywords: Astrophysics
    Type: GSFC-E-DAA-TN44055 , The Astrophysical Journal (ISSN 2041-8205) (e-ISSN 2041-8213); 835; 1; 65
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    NASA TECHNICAL REPORTS
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