Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
Herschel observations of the Centaurus cluster - the dynamics of cold gas in a cool core
MMTF-Ha and HST-FUV Imaging of the Filamentary Complex in ABELL 1795
Radio jet-ISM interaction and positive radio-mechanical feedback in Abell 1795
Star Formation Efficiency in the Cool Cores of Galaxy Clusters
The Nature of Filamentary Cold Gas in the Core of the Virgo Cluster
The Origins and Ionization Mechanisms of Halpha Filaments in the Cool Cores of Galaxy Groups and Clusters
Instrument
ACS, ACS/SBC
Temporal Coverage
2008-11-03T09:25:42Z/2009-02-27T08:04:44Z
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, Sparks comma William B., 2010, 'A Search for Ultraviolet Emission Filaments in Cool Core Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-nexq8kk