Testing Mass Determinations of Supermassive Black Holes via Stellar Kinematics

被引：14

作者：

Cappellari, Michele ^{[1
]}

McDermid, Richard M. ^{[1
]}

Bacon, R. ^{[1
]}

Davies, Roger L. ^{[1
]}

de Zeeuw, P. T. ^{[1
]}

Emsellem, Eric ^{[1
]}

Falcon-Barroso, Jesus ^{[1
]}

Krajnovic, Davor ^{[1
]}

Kuntschner, Harald ^{[1
]}

Peletier, Reynier F. ^{[1
]}

Sarzi, Marc ^{[1
]}

van den Bosch, Remco C. E. ^{[1
]}

van de Ven, Glenn ^{[1
]}

机构：

[1] Univ Oxford, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England

来源：

HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION | 2010年 / 1240卷

关键词：

GALAXY VELOCITY DISPERSION; TO-LIGHT RATIO; GALACTIC NUCLEI; SAURON PROJECT; LENTICULAR GALAXIES; MODELS; QUASARS; CENTERS; GROWTH; SIGMA;

D O I：

10.1063/1.3458489

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 MBH 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.

引用

页码：211 / +

页数：2

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