Comparison of Star Clusters With and Without Wolf-Rayet Stars in Wolf-Rayet Galaxies
From young massive star cluster to old globular: the LV-s0 relationship as a diagnostic tool
Gemini GMOS/IFU spectroscopy of NGC 1569 - I. Mapping the properties of a young star cluster and its environment
MEGARA-IFU detection of extended He II l4686 nebular emission in the central region of NGC 1569 and its ionization budget
The Resolved Stellar Population of the Poststarburst Galaxy NGC 1569
The Starburst-Interstellar Medium Interaction in NGC 1569. II. Small-Scale Examination of Nebular Emission, H II Region Size Distribution, and H II Region Luminosity Function
The Starburst-Interstellar Medium Interaction in NGC 1569. I. Location and Nature of HE II Sources UsingHubble Space Telescope WFPC2 Imagery
The Structure of the Super-Star Clusters in NGC 1569 from Hubble Space Telescope WFPC2 Images
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-01-10T05:30:15Z/1996-01-10T16:35:36Z
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, Leitherer comma Claus, 1997, 'NGC1569 AND NGC1705 AS LOCAL PROBES OF GALAXY EVOLUTION AT HIGH REDSHIFT', 1.0, European Space Agency, https://doi.org/10.5270/esa-m63ey1q