Compact Optical Counterparts of Ultraluminous X-Ray Sources
Compact Star Clusters in M81. I. Data from Hubble Space Telescope Wide Field Planetary Camera 2 Imaging
Compact Star Clusters in M81. II. Two Populations
Multiple Light Echoes from SN 1993J
Observability of Scattered-Light Echoes around Variable Stars and Cataclysmic Events
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Star Cluster Candidates in M81
The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space Telescope Imaging
The Progenitor of Supernova 1993J Revisited
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1995-01-31T10:34:17Z/1995-01-31T14:20:17Z
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, Kirshner comma Robert P., 1996, 'SINS: THE SUPERNOVA INTENSIVE STUDY - CYCLE4', 1.0, European Space Agency, https://doi.org/10.5270/esa-a8yklqk