An HST Study of Star Formation in Star-Burst Clusters
Photometric determination of the mass accretion rates of pre-main-sequence stars. VIII. Recent star formation in NGC 299
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. VI. The Case of LH 95 in the Large Magellanic Cloud
Pre-main sequence stars in LH 91
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2013-03-28T18:06:02Z/2013-09-29T20:53:41Z
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, De Marchi comma Guido, 2014, 'Studying pre-main sequence stars across the metallicity ladder', 1.0, European Space Agency, https://doi.org/10.5270/esa-5yoy7k7