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arXiv · 1001.3233

Testing Mass Determinations of Supermassive Black Holes via Stellar Kinematics

Michele Cappellari·Richard M. McDermid·R. Bacon·Roger L. Davies·P. T. de Zeeuw·Eric Emsellem·Jesus Falcon-Barroso·Davor Krajnovic·Harald Kuntschner·Reynier F. Peletier·Marc Sarzi·Remco C. E. van den Bosch·Glenn van de Ven
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Abstract

We investigate the accuracy of mass determinations M_BH of supermassive black holes in galaxies using dynamical models of the stellar kinematics. We compare 10 of our M_BH measurements, using integral-field OASIS kinematics, to published values. For a sample of 25 galaxies we confront our new M_BH derived using two modeling methods on the same OASIS data.

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Michele Cappellari, Richard M. McDermid, R. Bacon, Roger L. Davies, P. T. de Zeeuw, Eric Emsellem, Jesus Falcon-Barroso, Davor Krajnovic, Harald Kuntschner, Reynier F. Peletier, Marc Sarzi, Remco C. E. van den Bosch, Glenn van de Ven. 2010-01-19. Testing Mass Determinations of Supermassive Black Holes via Stellar Kinematics. https://doi.org/10.1063/1.3458489

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