A dataset provided by the European Space Agency

Name 6456
Title The photospheric iron abundance of UV bright stars in globular clusters
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6456;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-7gv0ylq
Author Napiwotzki, Ralf
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6456&mission=hst
Publication
  • Abundances of UV bright stars in globular clusters. I. ROA 5701 in omega Centauri and Barnard 29 in M 13
  • Iron abundances of B-type post-asymptotic giant branch stars in globular clusters: Barnard29 in M13 and ROA5701 in oCen
  • Observations of the Ultraviolet-bright Star Barnard 29 in the Globular Cluster M13 (NGC 6205)
Instrument HRS, HRS/2
Temporal Coverage 1996-08-03T21:16:04Z/1997-02-02T20:01:30Z
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 1998-02-03T22:40:14Z
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, Napiwotzki comma Ralf, 1998, 'The photospheric iron abundance of UV bright stars in globular clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-7gv0ylq