A dataset provided by the European Space Agency

Name 11980
Title Deep FUV Imaging of Cooling Flow Clusters
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=11980;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-34zzwmg
Author Veilleux, Sylvain
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=11980&mission=hst
Publication
  • Constraining star formation rates in cool-core brightest cluster galaxies
  • Far-ultraviolet morphology of star-forming filaments in cool core brightest cluster galaxies
  • HST-COS Spectroscopy of the Cooling Flow in A1795--Evidence for Inefficient Star Formation in Condensing Intracluster Gas
  • MMTF-Ha and HST-FUV Imaging of the Filamentary Complex in ABELL 1795
  • Star Formation Efficiency in the Cool Cores of Galaxy Clusters
  • Subaru Spectroscopy and Spectral Modeling of Cygnus A
  • The Origins and Ionization Mechanisms of Halpha Filaments in the Cool Cores of Galaxy Groups and Clusters
Instrument ACS, ACS/SBC
Temporal Coverage 2009-02-24T09:00:54Z/2009-05-04T21:27:57Z
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.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2010-05-05T01:24:03Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Veilleux comma Sylvain, 2010, 'Deep FUV Imaging of Cooling Flow Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-34zzwmg