An Optical Study of Stellar and Interstellar Environments of Seven Luminous and Ultraluminous X-Ray Sources
A Scattered Light Echo around SN 1993J in M81
A ULX in NGC 4559: a ``mini-cartwheel scenario?
Compact Optical Counterparts of Ultraluminous X-Ray Sources
Discovery of Five Candidate Analogs for e Carinae in Nearby Galaxies
Gaps in the Cloud Cover? Comparing Extinction Measures in Spiral Disks
Irradiation models for ULXs and fits to optical data
Multiple Light Echoes from SN 1993J
Nothing to see here: failed supernovae are faint or rare
Optical and infrared signatures of ultra-luminous X-ray sources
Optical Counterparts of the Nearest Ultraluminous X-Ray Sources
Probable intermediate-mass black holes in NGC 4559: XMM-Newton spectral and timing constraints
Properties of Resolved Star Clusters in M51
Recurring outbursts of the supernova impostor AT 2016blu in NGC 4559
The Globular Cluster Systems of Five Nearby Spiral Galaxies: New Insights from Hubble Space Telescope Imaging
The Opacity of Spiral Galaxy Disks. IV. Radial Extinction Profiles from Counts of Distant Galaxies Seen through Foreground Disks
The opacity of spiral galaxy disks. V. Dust opacity, HI distributions and sub-mm emission
The opacity of spiral galaxy disks. VI. Extinction, stellar light and color
The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
The opacity of spiral galaxy disks. VII. The accuracy of galaxy counts as an extinction probe
The Optical Counterpart of an Ultraluminous X-Ray Object in M81
The Progenitor of Supernova 1993J Revisited
The star-forming environment of an ultraluminous X-ray source in NGC4559: an optical study
The structure and environment of young stellar clusters in spiral galaxies
The Yellow Supergiant Progenitor of the Type II Supernova 2011dh in M51
Thick disks and halos of spiral galaxies M 81, NGC 55 and NGC 300
Ultra-luminous X-ray sources
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
2001-05-25T03:43:14Z/2001-06-09T18:27:34Z
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, Bregman comma Joel N., 2002, 'Ultraluminous X-Ray Sources and Intermediate Mass Black Holes', 1.0, European Space Agency, https://doi.org/10.5270/esa-75wl7kt