NuSTAR and Swift observations of Swift J1357.2-0933 during an early phase of its 2017 outburst
arXiv:1712.02804 · doi:10.3847/1538-4357/aa9d3e
Abstract
We present a detailed spectral analysis of Swift and NuSTAR observations of the very faint X-ray transient and black hole system Swift J1357.2-0933 during an early low hard state of its 2017 outburst. Swift J1357.2-0933 was observed at 0.02% of the Eddington luminosity (for a distance of 2.3 kpc and a mass of 4 M). Despite the low luminosity, the broadband X-ray spectrum between 0.3 and 78 keV requires the presence of a disk blackbody component with an inner disk temperature of T 0.06 keV in addition to a thermal Comptonization component with a photon index of Γ 1.70. Using a more physical model, which takes strong relativistic effects into account, and assuming a high inclination of 70, which is motivated by the presence of dips in optical light curves, we find that the accretion disk is truncated within a few RISCO from the black hole, independent of the spin.
arXiv comment11 pages, 5 figures, accepted for publication in ApJ
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Cited by in corpus (4)
- The black hole X-ray transient Swift J1357.2-0933 as seen with Swift and NuSTAR during its 2017 outburst
- Puzzling Blue Dips in the Black Hole Candidate Swift J1357.2-0933, from ULTRACAM, SALT, ATCA, Swift and NuSTAR
- Implications on accretion flow dynamics from spectral study of Swift~J1357.2-0933
- Global Accretion Properties of Black Hole X-Ray Binaries: A Phenomenological Perspective