Connections between Star Cluster Populations and Their Host Galaxy Nuclear Rings
Measuring the Mass of the Central Black Hole in the Bulgeless Galaxy NGC 4395 from Gas Dynamical Modeling
Modeling the Spectral Energy Distribution of the Active Galactic Nucleus inside NGC 4395
Resolved Nuclear Kinematics Link the Formation and Growth of Nuclear Star Clusters with the Evolution of Their Early- and Late-type Hosts
The Off-centered Seyfert-like Compact Emission in the Nuclear Region of NGC 3621
The Red Supergiant Progenitor of Type II Supernova 2024ggi
The Structure of Nuclear Star Clusters in Nearby Late-type Spiral Galaxies from Hubble Space Telescope Wide Field Camera 3 Imaging
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-10-07T13:23:30Z/2011-08-08T04:30:04Z
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, Barth comma Aaron J., 2012, 'Structure and Stellar Content of the Nearest Nuclear Clusters in Late-Type Spiral Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-32vymzo
