Angular momentum of z ~ 1.5 galaxies and their local analogues with adaptive optics
CO Excitation in High-z Main-sequence Analogues: Resolved CO(4-3)/CO(3-2) Line Ratios in DYNAMO Galaxies
Connecting Clump Sizes in Turbulent Disk Galaxies to Instability Theory
DYNAMO-HST survey: clumps in nearby massive turbulent discs and the effects of clump clustering on kiloparsec scale measurements of clumps
DYNAMO - II. Coupled stellar and ionized-gas kinematics in two low-redshift clumpy discs
Extreme Gas Fractions in Clumpy, Turbulent Disk Galaxies at z ~ 0.1
Integrated and resolved dust attenuation in clumpy star-forming galaxies at 0.07 < z < 0.14
Low Angular Momentum in Clumpy, Turbulent Disk Galaxies
Robust Cross-correlation-based Measurement of Clump Sizes in Galaxies
Size Scaling of Clump Instabilities in Turbulent, Feedback-regulated Disks
Stellar masses of clumps in gas-rich, turbulent disc galaxies
Systematic Difference between Ionized and Molecular Gas Velocity Dispersions in z ~ 1-2 Disks and Local Analogs
Testing Feedback-regulated Star Formation in Gas-rich, Turbulent Disk Galaxies
The connection between the peaks in velocity dispersion and star-forming clumps of turbulent galaxies
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC
Temporal Coverage
2013-03-19T02:10:37Z/2013-07-19T04:51:56Z
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, Damjanov comma Ivana, 2014, 'Local Turbulent Disks: analogs of high-redshift vigorously star-forming disks and laboratories for galaxy assembly?', 1.0, European Space Agency, https://doi.org/10.5270/esa-kwni9ea