History and destiny of an emerging early-type galaxy. New IFU insights on the major-merger remnant NGC 7252
Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case
Luminosity profiles and sizes of massive star clusters in NGC 7252
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2010-07-29T15:40:00Z/2010-07-29T18:01:55Z
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, Bastian comma Nate, 2011, 'Luminosity Profiles of Extremely Massive Clusters in NGC 7252', 1.0, European Space Agency, https://doi.org/10.5270/esa-ihf4awq