A Correlation between Galaxy Light Concentration and Supermassive Black Hole Mass
A Log-Quadratic Relation for Predicting Supermassive Black Hole Masses from the Host Bulge Sersic Index
Are Nuclear Star Clusters the Precursors of Massive Black Holes?
A Strong Correlation between Circumnuclear Dust and Black Hole Accretion in Early-Type Galaxies
Bar-driven evolution of S0s: the edge-on galaxy NGC 4570
Counting the Unseen. I. Nuclear Density Scaling Relations for Nucleated Galaxies
Detection of Enhanced Central Mass-to-light Ratios in Low-mass Early-type Galaxies: Evidence for Black Holes?
Efficient multi-Gaussian expansion of galaxies
Evidence for a Massive Black Hole in the S0 Galaxy NGC 4342
Multiband photometric decomposition of nuclear stellar disks
Nuclear stellar discs in early-type galaxies - I. HST and WHT observations
Six new supermassive black hole mass determinations from adaptive-optics assisted SINFONI observations
Structure and Formation of Elliptical and Spheroidal Galaxies
The ATLAS3D Project - XXIII. Angular momentum and nuclear surface brightness profiles
The SAURON Project - XIV. No escape from Vesc: a global and local parameter in early-type galaxy evolution
Virial models and anisotropy of velocity dispersion in E-galaxies
Instrument
FOS/RD, WFPC2, WFPC2/PC
Temporal Coverage
1996-01-21T20:47:16Z/1996-05-09T09:33:35Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Jaffe comma Walter, 1997, 'DYNAMICS AND AGES OF NUCLEAR STELLAR DISKS IN VIRGO E/S0 GALAXIES', 1.0, European Space Agency, https://doi.org/10.5270/esa-plli8kh
