Laboratory atomic spectroscopy for the FUSE mission

Glenn Wahlgren, Hampus Nilsson, Stefan Ivarsson, Sveneric Johansson

Research output: Chapter in Book/Report/Conference proceedingPaper in conference proceedingpeer-review

Abstract

Spectra of hot (type B) stars obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) satellite in the region 1000-1200
Original languageEnglish
Title of host publication8th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (ASOS 8)
PublisherUniv. of Wisconsin
PagesT18-T18
Publication statusPublished - 2004
Event8th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (ASOS 8) - Madison, WI, United States
Duration: 2004 Aug 82004 Aug 12

Conference

Conference8th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (ASOS 8)
Country/TerritoryUnited States
CityMadison, WI
Period2004/08/082004/08/12

Subject classification (UKÄ)

  • Astronomy, Astrophysics and Cosmology

Free keywords

  • Fe
  • Cr
  • 1000 to 1200 Å
  • 3d-4f transition
  • optical wavelength
  • Fe II transition
  • oscillator strength
  • vacuum echelle spectrometer
  • missing opacity
  • spectral line
  • Fe II/III
  • metal-rich stellar atmosphere
  • Cr II/III
  • synthetically calculated spectra
  • spectral fitting
  • Far Ultraviolet Spectroscopic Explorer satellite
  • type B stars
  • hot stars
  • stellar spectra
  • laboratory atomic spectroscopy
  • FUSE mission

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