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19 April 2024
 
  » arxiv » 1310.3830

 Article overview


The Reflection Component from Cygnus X-1 in the Soft State Measured by NuSTAR and Suzaku
John A. Tomsick ; Michael A. Nowak ; Michael Parker ; Jon M. Miller ; Andy C. Fabian ; Fiona A. Harrison ; Matteo Bachetti ; Didier Barret ; Steven E. Boggs ; Finn E. Christensen ; William W. Craig ; Karl Forster ; Felix Fuerst ; Brian W. Grefenstette ; Charles J. Hailey ; Ashley L. King ; Kristin K. Madsen ; Lorenzo Natalucci ; Katja Pottschmidt ; Randy R. Ross ; Daniel Stern ; Dominic J. Walton ; Joern Wilms ; William W. Zhang ;
Date 14 Oct 2013
AbstractThe black hole binary Cygnus X-1 was observed in late-2012 with the Nuclear Spectroscopic Telescope Array (NuSTAR) and Suzaku, providing spectral coverage over the ~1-300 keV range. The source was in the soft state with a multi-temperature blackbody, power-law, and reflection components along with absorption from highly ionized material in the system. The high throughput of NuSTAR allows for a very high quality measurement of the complex iron line region as well as the rest of the reflection component. The iron line is clearly broadened and is well-described by a relativistic blurring model, providing an opportunity to constrain the black hole spin. Although the spin constraint depends somewhat on which continuum model is used, we obtain a*>0.83 for all models that provide a good description of the spectrum. However, none of our spectral fits give a disk inclination that is consistent with the most recently reported binary values for Cyg X-1. This may indicate that there is a >13 degree misalignment between the orbital plane and the inner accretion disk (i.e., a warped accretion disk) or that there is missing physics in the spectral models.
Source arXiv, 1310.3830
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