The black hole in NGC 3379: a comparison of gas and stellar dynamical mass measurements with HST and integral-field data
Open Access
- 22 June 2006
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 370 (2) , 559-579
- https://doi.org/10.1111/j.1365-2966.2006.10537.x
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This publication has 61 references indexed in Scilit:
- The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and DistancesThe Astrophysical Journal, 2001
- The Shape and Orientation of NGC 3379: Implications for Nuclear DecouplingThe Astronomical Journal, 2001
- Stellar dynamics in the Galactic Centre: proper motions and anisotropyMonthly Notices of the Royal Astronomical Society, 2000
- A Fundamental Relation between Supermassive Black Holes and Their Host GalaxiesThe Astrophysical Journal, 2000
- A Photometric and Kinematic Study of the Stars and Interstellar Medium in the Central 2 Kiloparsecs of NGC 3379The Astrophysical Journal, 2000
- Evolutionary Stellar Population Synthesis at 2 A Spectral ResolutionThe Astrophysical Journal, 1999
- The Stellar Kinematic Fields of NGC 3379The Astronomical Journal, 1999
- High Proper‐Motion Stars in the Vicinity of Sagittarius A*: Evidence for a Supermassive Black Hole at the Center of Our GalaxyThe Astrophysical Journal, 1998
- The dynamical evolution of massive black hole binaries — II. Self-consistent N-body integrationsNew Astronomy, 1997
- Triaxial equilibrium models for elliptical galaxies with slow figure rotationThe Astrophysical Journal, 1982