A dataset provided by the European Space Agency

Name 5495
Title UV EMISSION LINE FORMATION PROCESSES AROUND THE BRIGHTEST HERBIG AE STAR HD104237 CYCLE 4 - MED
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=5495;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-fn2jpew
Author Brown, Alexander
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=5495&mission=hst
Publication
  • Identification of Fe II Emission Lines in FUSE Stellar Spectra
  • The Environment of the Optically Brightest Herbig Ae Star, HD 104237
Instrument HRS, HRS/1, HRS/2
Temporal Coverage 1994-11-07T08:20:17Z/1994-11-07T15:06:15Z
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 1995-11-07T23:45:14Z
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, Brown comma Alexander, 1995, 'UV EMISSION LINE FORMATION PROCESSES AROUND THE BRIGHTEST HERBIG AE STAR HD104237 CYCLE 4 - MED', 1.0, European Space Agency, https://doi.org/10.5270/esa-fn2jpew