A Spectroscopic Study of Component C and the Extended Emission around I Zw 18
Chandra Observations of the Three Most Metal Deficient Blue Compact Dwarf Galaxies Known in the Local Universe, SBS 0335-052, SBS 0335-052W, and I Zw 18
Isolating Clusters with Wolf-Rayet Stars in I Zw 18
New Light on the Stellar Populations in I Zw 18: Deep Near-Infrared Imaging
Observations of Starburst Galaxies With Far-Ultraviolet Spectrographic Explorer: Galactic Feedback in the Local Universe
Photometric studies of very metal-deficient blue compact dwarf galaxies: the exponential ionized gas halo of IZw18
Searching for Wolf-Rayet Stars in I ZW 18: the Origin of He II Emission
Spatial Distribution and Evolution of the Stellar Populations and Candidate Star Clusters in the Blue Compact Dwarf I Zwicky 18
Spatially resolved integral field spectroscopy of the ionized gas in IZw18
Structural Properties of Massive Young Clusters
Testing Models for Molecular Gas Formation in Galaxies: Hydrostatic Pressure or Gas and Dust Shielding?
The Complex Kinematics of the Neutral Hydrogen Associated with I ZW 18
The Massive Stars of I ZW 18 as Seen in Hubble Space Telescope Images
The Star Formation History of I ZW 18
What heats the bright H II regions in I ZW 18?
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1994-10-29T22:34:17Z/1994-11-03T05:33:37Z
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, HUNTER DEIDRE, 1995, 'STAR FORMATION AND THE MASSIVE STAR POPULATION IN BLUE COMPACT DWARF GALAXIES: CYCLE4MEDIUM', 1.0, European Space Agency, https://doi.org/10.5270/esa-m6etreh