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arXiv · 0709.2861

Supermassive black holes from OASIS and SAURON integral-field kinematics

M. Cappellari·R. Bacon·R. L. Davies·P. T. de Zeeuw·E. Emsellem·J. Falcon-Barroso·D. Krajnovic·H. Kuntschner·R. M. McDermid·R. F. Peletier·M. Sarzi·R. C. E. van den Bosch·G. van de Ven
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Abstract

Supermassive black holes are a key element in our understanding of how galaxies form. Most of the progress in this very active field of research is based on just ~30 determinations of black hole mass, accumulated over the past decade. We illustrate how integral-field spectroscopy, and in particular our OASIS modeling effort, can help improve the current situation.

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M. Cappellari, R. Bacon, R. L. Davies, P. T. de Zeeuw, E. Emsellem, J. Falcon-Barroso, D. Krajnovic, H. Kuntschner, R. M. McDermid, R. F. Peletier, M. Sarzi, R. C. E. van den Bosch, G. van de Ven. 2007-09-18. Supermassive black holes from OASIS and SAURON integral-field kinematics. https://doi.org/10.1017/s1743921308017687

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