Giant star-forming complexes in high-z main-sequence galaxy analogues: the internal structure of clumps in DYNAMO galaxies
K-band Imaging of the Nearby Clumpy, Turbulent Disk Galaxy DYNAMO G04-1
Stellar masses of clumps in gas-rich, turbulent disc galaxies
Instrument
WFC3/IR, WFC3/UVIS
Temporal Coverage
2018-02-26T10:15:26Z/2018-11-04T06:20:43Z
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, Fisher et al., 2019, 'The ages and baryonic masses of clumps in turbulent, clumpy disk galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-z4cnrsj