Axisymmetric, three-integral models of galaxies: A massive black hole in NGC 3379

We fit axisymmetric three-integral dynamical models to NGC 3379 using the line-of-sight velocity distribution obtained from Hubble Space Telescope FOS spectra of the galaxy center and ground-based long-slit spectroscopy along four position angles, with the light distribution constrained by WFPC2 and...

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Dettagli Bibliografici
Autori principali: Gebhardt, K, Richstone, D, Kormendy, J, Lauer, T, Ajhar, E, Bender, R, Dressler, A, Faber, S, Grillmair, C, Magorrian, J, Tremaine, S
Natura: Journal article
Lingua:English
Pubblicazione: 2000

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