A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole
Charge exchange in the ultraviolet: implication for interacting clouds in the core of NGC 1275
Cold, clumpy accretion onto an active supermassive black hole
Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
Herschel observations of extended atomic gas in the core of the Perseus cluster
HST/STIS Far-UV observations of the central nebulae in the cooling core cluster A 1795
Hubble Space Telescope STIS Far-Ultraviolet Observations of the Central Nebulae in the Cooling-Core Clusters A1795 and A2597
Hubble Space Telescope STIS Spectroscopy of the Lya Emission Line in the Central Dominant Galaxies in A426, A1795, and A2597: Constraints on Clouds in the Intracluster Medium
Jet-Cloud Interactions in Compact Radio Sources
Residual cooling and persistent star formation amid active galactic nucleus feedback in Abell 2597
Instrument
STIS, STIS/CCD, STIS/FUV-MAMA
Temporal Coverage
2000-01-17T11:35:49Z/2001-03-17T19:23:43Z
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, ODea comma Christopher P., 2006, 'What is the Nature of the Cold Medium in Cooling Flow Clusters? Clues from L-alpha', 1.0, European Space Agency, https://doi.org/10.5270/esa-f0xzk0m