The browser you are using is not supported by this website. All versions of Internet Explorer are no longer supported, either by us or Microsoft (read more here: https://www.microsoft.com/en-us/microsoft-365/windows/end-of-ie-support).

Please use a modern browser to fully experience our website, such as the newest versions of Edge, Chrome, Firefox or Safari etc.

Laboratory atomic spectroscopy for the FUSE mission

På svenska

Author

Summary, in English

Spectra of hot (type B) stars obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) satellite in the region 1000-1200

Publishing year

2004

Language

English

Pages

18-18

Publication/Series

8th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (ASOS 8)

Document type

Conference paper

Publisher

Univ. of Wisconsin

Topic

  • Astronomy, Astrophysics and Cosmology

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

Conference name

8th International Colloquium on Atomic Spectra and Oscillator Strengths for Astrophysical and Laboratory Plasmas (ASOS 8)

Conference date

2004-08-08 - 2004-08-12

Conference place

Madison, WI, United States

Status

Published