First Constraints on Black Hole Spin in Broad Iron Line AGN

Astronomy and Astrophysics – Astronomy

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Scientific paper

Black holes are arguably the simplest objects in nature, with an ability to be completely defined by two mathematical quantities: mass and spin. Spin, being a general relativistic effect, is the more difficult to discern of the two. One of the most promising and robust methods for constraining this quantity relies on modeling the relativistically altered shape of the iron-K line emitted from the accretion disk around the black hole. With this in mind, I have expanded upon previous emission line model codes to create a new relativistic emission line model, called kerrdisk, which allows the black hole spin to be fit as a free parameter. This allows us to robustly constrain the angular momentum of a black hole for the first time. Herein I present the results of spectral fitting of this model to several AGN with robustly observed broad iron lines in an effort to perform the very first statistically robust study of black hole spin distribution in these types of sources. This is a crucial first step toward taking a census of black hole spin in both AGN and GBHCs.
I gratefully acknowledge funding from NSF grant AST0205990, which has contributed to this research.

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