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2006MNRAS.367....2H - Mon. Not. R. Astron. Soc., 367, 2-18 (2006/March-3)
The central kinematics of NGC 1399 measured with 14 pc resolution.
HOUGHTON R.C.W., MAGORRIAN J., SARZI M., THATTE N., DAVIES R.L. and KRAJNOVIC D.
Abstract (from CDS):
We use spherical orbit-superposition models to interpret the kinematics, using a set of orthogonal `eigen-velocity profiles' that allow us to fit models directly to spectra. The models require a central black hole of mass 1.2+0.5–0.6x 109 M☉, with a strongly tangentially biased orbit distribution in the inner 40pc.
Abstract Copyright: 2006 The Authors.Journal compilation © 2006 RAS
Journal keyword(s): instrumentation: adaptive optics - galaxies: individual: NGC 1399 - galaxies: kinematics and dynamics
Simbad objects: 12
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