Physical conditions in the gas phases of the giant H II region LMC-N 11 unveiled by Herschel . I. Diffuse C II and O III emission in LMC-N 11B
Pre-main sequence stars in the stellar association N11 in the Large Magellanic Cloud
Pre-main-sequence stars in the stellar association N 11 in the Large Magellanic Cloud: clustering properties
The effects of star formation on the low-metallicity ISM: NGC 4214 mapped with Herschel/PACS spectroscopy
The impact of satellite trails on Hubble Space Telescope observations
The Young Stellar Population of NGC 4214 as Observed with the Hubble Space Telescope. I. Data and Methods
The Young Stellar Population of NGC 4214 as Observed with the Hubble Space Telescope. II. Results
X-Shooting ULLYSES: Massive stars at low metallicity: X. Physical parameters and feedback of massive stars in the LMC N11 B star-forming region
Instrument
ACS, ACS/HRC, ACS/WFC
Temporal Coverage
2002-12-27T08:17:20Z/2003-11-26T23:42:12Z
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, Maiz Apellaniz et al., 2004, 'The Complete IMF of a Massive Young Cluster', 1.0, European Space Agency, https://doi.org/10.5270/esa-r0m4bz4
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.