A Hubble Space Telescope Study of Star Formation in the Inner Resonance Ring of NGC 3081
Co-evolution of nuclear rings, bars and the central intensity ratio of their host galaxies
Connections between Star Cluster Populations and Their Host Galaxy Nuclear Rings
The Inner Resonance Ring of NGC 3081. II. Star Formation, Bar Strength, Disk Surface Mass Density, and Mass-to-Light Ratio
The Ringed Spiral Galaxy NGC4622. II. An Independent Determination that the Two Outer Arms Lead
The Ringed Spiral Galaxy NGC 4622. I. Photometry, Kinematics, and the Case for Two Strong Leading Outer Spiral Arms
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2000-06-23T22:29:14Z/2001-05-25T21:56:34Z
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, Buta comma Ronald, 2002, 'A Study of Star Formation in Galactic Resonance Rings', 1.0, European Space Agency, https://doi.org/10.5270/esa-azapk0f