A Possible High Nova Rate for Two Local Group Dwarf Galaxies: M32 and NGC 205
Evolution of Nuclear Star Clusters
Improved Dynamical Constraints on the Masses of the Central Black Holes in Nearby Low-mass Early-type Galactic Nuclei and the First Black Hole Determination for NGC 205
The impact of satellite trails on Hubble Space Telescope observations
The Low End of the Supermassive Black Hole Mass Function: Constraining the Mass of a Nuclear Black Hole in NGC 205 via Stellar Kinematics
The young stellar population at the center of NGC 205
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, Ferrarese et al., 2003, 'Nuclear Dynamics of NGC 205: Probing the Low-Mass End of the M-sigma Relation', 1.0, European Space Agency, https://doi.org/10.5270/esa-x7xmsrt