NuSTARand Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays

M. L. Parker, J. A. Tomsick, J. A. Kennea, J. M. Miller, F. A. Harrison, D. Barret, S. E. Boggs, Finn Erland Christensen, W. W. Craig, A. C. Fabian, F. Fürst, V. Grinberg, C. J. Hailey, P. Romano, D. Stern, D. J. Walton, W. W. Zhang

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Abstract

We present results from spectral fitting of the very high state of GX 339-4 with Nuclear Spectroscopic Telescope Array (NuSTAR) and Swift. We use relativistic reflection modeling to measure the spin of the black hole and inclination of the inner disk and find a spin of a = 0.95(-0.08)(+0.02) and inclination of 30 degrees +/- 1 degrees (statistical errors). These values agree well with previous results from reflection modeling. With the exceptional sensitivity of NuSTAR at the high-energy side of the disk spectrum, we are able to constrain multiple physical parameters simultaneously using continuum fitting. By using the constraints from reflection as input for the continuum fitting method, we invert the conventional fitting procedure to estimate the mass and distance of GX 339-4 using just the X-ray spectrum, finding a mass of 9.0(-1.2)(+1.6) M-circle dot and distance of 8.4 +/- 0.9 kpc (statistical errors).
Original languageEnglish
Article numberL6
JournalThe Astrophysical Journal. Letters
Volume821
Issue number1
Number of pages6
ISSN2041-8205
DOIs
Publication statusPublished - 2016

Keywords

  • X-ray binaries
  • Stellar radiation and spectra
  • black holes
  • statistical analysis
  • stellar spectra
  • X-ray binary stars
  • X-ray spectra
  • spectral fitting
  • Nuclear Spectroscopic Telescope Array observation data
  • Swift observation data
  • relativistic reflection modeling
  • black hole spin
  • statistical errors
  • disk spectrum
  • physical parameters
  • continuum fitting method
  • X-ray spectrum

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