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Monte Carlo simulations of dusty gas discs around supermassive black holes

Published online by Cambridge University Press:  01 August 2006

Maarten Baes
Affiliation:
Universiteit Gent, Belgium, email: [email protected]
Sławomir Piasecki
Affiliation:
Universiteit Gent, Belgium, email: [email protected] Adam Mickiewicz University, Poznań, Poland
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Abstract

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Using detailed Monte Carlo radiative transfer simulations in realistic models for galactic nuclei, we critically investigate the influence of interstellar dust in ionised gas discs on the rotation curves and the resulting black hole mass measurements. We find that absorption and scattering by interstellar dust leaves the shape of the rotation curves basically unaltered, but slightly decreases the central slope of the rotation curves. As a result, the “observed” black hole masses are systematically underestimated by some 10 to 20% for realistic optical depths.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Atkinson, J. W., Collett, J. L., Marconi, A. et al. 2005, MNRAS, 359, 504CrossRefGoogle Scholar
Baes, M. & Dejonghe, H. 2002, MNRAS, 335, 441CrossRefGoogle Scholar
Baes, M., Davies, J. I., Dejonghe, H. et al. 2003, MNRAS, 343, 1081CrossRefGoogle Scholar
Barth, A. J., Sarzi, M., Rix, H.-W. et al. 2001, ApJ, 555, 685CrossRefGoogle Scholar
Häring-Neumayer, N., Cappellari, M., Rix, H.-W. et al. 2006, ApJ, 643, 226CrossRefGoogle Scholar
Marconi, A., Axon, D. J., Capetti, A. et al. 2003, ApJ, 586, 868CrossRefGoogle Scholar