A dataset provided by the European Space Agency

Name 9300
Title Starburst Galaxies and Their Population of Super Star Clusters
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=9300;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-sghgyt5
Author Ford, Holland
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=9300&mission=hst
Publication
  • Anatomy of a young massive star cluster: NGC 1569-B
  • Chemical composition of the young massive cluster NGC 1569-B
  • Evidence for the strong effect of gas removal on the internal dynamics of young stellar clusters
  • Far-ultraviolet Observations of Outflows from Infrared-luminous Galaxies
  • Gemini GMOS/IFU spectroscopy of NGC 1569 - I. Mapping the properties of a young star cluster and its environment
  • On the fraction of star clusters surviving the embedded phase
  • Resolved photometry of extragalactic young massive star clusters
  • Resolving Extragalactic Star Clusters with HST/ACS
  • Star cluster formation in the most extreme environments: insights from the HiPEEC survey
  • The nearest extreme starburst: bubbles, young star clusters and outflow in the merger NGC 3256
Instrument ACS, ACS/HRC
Temporal Coverage 2002-08-05T18:43:00Z/2002-09-04T05:03:46Z
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 2003-09-05T21:06:55Z
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, Ford et al., 2003, 'Starburst Galaxies and Their Population of Super Star Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-sghgyt5