Dwarf Galaxies in Clusters as Probes of Galaxy Formation and Dark Matter
Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
Filamentary star formation in NGC 1275
Herschel observations of extended atomic gas in the core of the Perseus cluster
Hydrogen two-photon continuum emission from the Horseshoe filament in NGC 1275
Magnetic support of the optical emission line filaments in NGC 1275
Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. I. Spiral Disk
The ALMA Discovery of the Rotating Disk and Fast Outflow of Cold Molecular Gas in NGC 1275
The energy source of the filaments around the giant galaxy NGC 1275
Instrument
ACS/SBC, WFPC2, WFPC2/PC
Temporal Coverage
2008-03-16T05:37:11Z/2008-03-21T05:59:57Z
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, OConnell comma Robert W., 2009, 'Star Formation in the Perseus Cluster Cooling Flow', 1.0, European Space Agency, https://doi.org/10.5270/esa-rhajmb5