The implications of the X-ray emission patterns of galaxies hosting supermassive black holes have been contentious. Data from NASA's NuSTAR telescope seem to resolve the issue — at least for one such galaxy. See Letter p.449
References
Risaliti, G. et al. Nature 494, 449–451 (2013).
Volonteri, M., Madau, P., Quataert, E. & Rees, M. J. Astrophys. J. 620, 69–77 (2005).
King, A. R. & Pringle, J. E. Mon. Not. R. Astron. Soc. 373, L90–L92 (2006).
Tanaka, Y. et al. Nature 375, 659–661 (1995).
Fabian, A. C. et al. Mon. Not. R. Astron. Soc. 277, L11–L15 (1995).
Miller, J. M. et al. Astrophys. J. 606, L131–L134 (2004).
Brenneman, L. W. & Reynolds, C. S. Astrophys. J. 652, 1028–1043 (2006).
Miller, L., Turner, T. J. & Reeves J. N. Astron. Astrophys. 483, 437–452 (2008).
Reynolds, C. S. et al. Mon. Not. R. Astron. Soc. 397, L21–L25 (2009).
Reynolds, C. S. Astrophys. J. 759, L15 (2012).
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Reynolds, C. Black holes in a spin. Nature 494, 432–433 (2013). https://doi.org/10.1038/494432a
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DOI: https://doi.org/10.1038/494432a
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