Boroson and Lauer reply

Todd A. Boroson () and Tod R. Lauer ()
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Todd A. Boroson: National Optical Astronomy Observatory
Tod R. Lauer: National Optical Astronomy Observatory

Nature, 2010, vol. 463, issue 7277, E2-E2

Abstract: Abstract Replying to: C. M. Gaskell Nature 463, 10.1038/nature08665 (2010) Gaskell1 makes the point that the profile of the Balmer lines in the candidate binary supermassive black hole2 AGN J1536+0441 bears some similarity to those that are thought to arise from disk emission in other objects. He further argues that two predictions of the competing binary black-hole hypothesis are (1) radial velocity changes that are interpretable in terms of the binary orbit, and (2) line fluxes in the two peaks that vary independently.

Date: 2010
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DOI: 10.1038/nature08666

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