A ~15 kpc outflow cone piercing through the halo of the blue compact metal-poor galaxy SBS 0335-052E
a New View of the Super Star Clusters in the Low-Metallicity Galaxy SBS 0335-052
A robust measurement of the mass outflow rate of the galactic outflow from NGC 6090
Detection of H I in Emission in the LYa Emitting Galaxy Haro 11
DUVET: Spatially Resolved Observations of Star Formation Regulation via Galactic Outflows in a Starbursting Disk Galaxy
Exploring the Overabundance of ULXs in Metal- and Dust-poor Local Lyman Break Analogs
Extreme Variation in Star Formation Efficiency across a Compact, Starburst Disk Galaxy
Far-ultraviolet Observations of Outflows from Infrared-luminous Galaxies
Haro 11 - Untying the knots of the nuclear starburst
Haro 11: Where is the Lyman Continuum Source?
HI in very metal-poor galaxies: the SBS 0335-052 system
Hubble Space Telescope Morphologies of Local Lyman Break Galaxy Analogs. I. Evidence for Starbursts Triggered by Merging
Kinematics of Haro 11: The miniature Antennae
Molecular depletion times and the CO-to-H2 conversion factor in metal-poor galaxies
Neutral gas in Lyman-alpha emitting galaxies Haro 11 and ESO 338-IG04 measured through sodium absorption
On the detectability of Lya emission in star forming galaxies. The role of dust
On the Origin of the Red Excess in Very Young Super Star Clusters: The Case of SBS 0335-052E
On the properties of the interstellar medium in extremely metal-poor blue compact dwarf galaxies. A VIMOS-IFU study of the cometary galaxy and Ly a absorber Tol 65
Physical properties and evolutionary state of the Lyman alpha emitting starburst galaxy IRAS 08339+6517
Probing cluster formation under extreme conditions: massive star clusters in blue compact galaxies
Probing Star Formation at Low Metallicity: The Radio Emission of Super Star Clusters in SBS 0335-052
Star formation histories in mergers: the spatially resolved properties of the early-stage merger luminous infrared galaxies IC 1623 and NGC 6090
Stars and gas in the most metal-poor galaxies - I. COS and MUSE observations of SBS 0335-052E
Super star clusters in Haro 11: properties of a very young starburst and evidence for a near-infrared flux excess
Super Star Clusters in SBS0335-052E
Testing Models for Molecular Gas Formation in Galaxies: Hydrostatic Pressure or Gas and Dust Shielding?
The Contribution of Host Galaxies to the Infrared Energy Output of z 5.0 Quasars
The escape of Lyman photons from a young starburst: the case of Haro11+
The impact of satellite trails on Hubble Space Telescope observations
The impact of stellar feedback from velocity-dependent ionized gas maps - a MUSE view of Haro 11
The Lyman Alpha Morphology of Local Starburst Galaxies: Release of Calibrated Images
The Lyman Alpha Reference Sample: Extended Lyman Alpha Halos Produced at Low Dust Content
The Lyman Alpha Reference Sample. III. Properties of the Neutral ISM from GBT and VLA Observations
The Lya Reference Sample. XIV. Lya Imaging of 45 Low-redshift Star-forming Galaxies and Inferences on Global Emission
The nature of the interstellar medium of the starburst low-metallicity galaxy Haro 11: a multi-phase model of the infrared emission
The Source of Leaking Ionizing Photons from Haro11: Clues from HST/COS Spectroscopy of Knots A, B, and C
ULX contribution to stellar feedback: an intermediate-mass black hole candidate and the population of ULXs in the low-metallicity starburst galaxy ESO 338-4
VLT/MUSE illuminates possible channels for Lyman continuum escape in the halo of SBS 0335-52E
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2005-11-12T12:50:00Z/2006-08-22T02:25:25Z
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, Oestlin et al., 2007, 'Lyman alpha morphology of local starburst galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-ej7l2pe