Astronomy and Astrophysics – Astrophysics
Scientific paper
2007-10-17
Astronomy and Astrophysics
Astrophysics
5 pages, 2 figures, to appear in the proceedings of IAUS 246, "Dynamical Evolution of Dense Stellar Systems", ed. Vesperini, G
Scientific paper
10.1017/S1743921308015883
We present optical and X-ray data for the first object showing strong evidence for being a black hole in a globular cluster. We show the initial X-ray light curve and X-ray spectrum which led to the discovery that this is an extremely bright, highly variable source, and thus must be a black hole. We present the optical spectrum which unambiguously identifies the optical counterpart as a globular cluster, and which shows a strong, broad [O III] emission line, most likely coming from an outflow driven by the accreting source.
Bergond Gilles
Kundu Arunav
Maccarone Thomas J.
Rhode Katherine L.
Salzer John Joseph
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