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...
主要な著者: | Gebhardt, K, Richstone, D, Kormendy, J, Lauer, T, Ajhar, E, Bender, R, Dressler, A, Faber, S, Grillmair, C, Magorrian, J, Tremaine, S |
---|---|
フォーマット: | Journal article |
言語: | English |
出版事項: |
2000
|
類似資料
-
Spectroscopic evidence for a supermassive black hole in NGC 4486B
著者:: Kormendy, J, 等
出版事項: (1997) -
The demography of massive dark objects in galaxy centers
著者:: Magorrian, J, 等
出版事項: (1998) -
Axisymmetric dynamical models of the central regions of galaxies
著者:: Gebhardt, K, 等
出版事項: (2003) -
Supermassive black holes and the evolution of galaxies
著者:: Richstone, D, 等
出版事項: (1998) -
A STELLAR DYNAMICAL MEASUREMENT OF THE BLACK HOLE MASS IN THE MASER GALAXY NGC 4258
著者:: Siopis, C, 等
出版事項: (2009)