Hostname: page-component-77c89778f8-5wvtr Total loading time: 0 Render date: 2024-07-17T15:47:13.869Z Has data issue: false hasContentIssue false
  • English
  • Français

A Photospheric Solar Iron Abundance from Weak FeII Lines

Published online by Cambridge University Press:  19 July 2016

U. Pauls ,
N. Grevesse  and
M. C. E. Huber
U. Pauls
Affiliation:
Institut für Astronomie, Eidgenössische Technische Hochschule, ETH–Zentrum CH – 8092 Zürich, Switzerland
N. Grevesse
Affiliation:
Institut d'Astrophysique, Université de Liège, B – 4200 Ougrée–Liège, Belgium
M. C. E. Huber
Affiliation:
Institut für Astronomie, Eidgenössische Technische Hochschule, ETH–Zentrum CH – 8092 Zürich, Switzerland

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The high resolution and the high light-gathering power of a Fourier–transform spectrometer (FTS) afford the observation of very weak lines in laboratory spectra. Thus it became possible to determine an accurate solar iron abundance from Fe II lines that are weak in the solar spectrum: we measured the branching fractions of a few such lines whose upper levels lifetimes are known.

Type
VI. Chemical Composition of Stars
Information
Symposium - International Astronomical Union , Volume 132: The Impact of Veryhigh S/N Spectroscopy on Stellar Physics , 1988 , pp. 425 - 427
Copyright
Copyright © Kluwer 1988 

References

Adams, DL & Whaling, W 1981 J. Opt. Soc. Am. 71 1036–1038 Google Scholar
Brault, JW 1985 in High Resolution in Astronomy 15thAdvanced Course of the Swiss Society of Astronomy and Astrophysics, Saas-Fee (Sauverny: Obs. de Genève) pp 1–61 Google Scholar
Grevesse, N 1984a Phys. Scripta T8 49–58 Google Scholar
Grevesse, N 1984b in Frontiers of Astronomy and Astrophysics Proceedings of the 7th European Regional Astronomy Meeting (Firenze: Italian Astron. Soc.) pp 72–81 Google Scholar
Hannaford, P & Lowe, R 1983 J. Phys. B: At. Mol. Phys. 16 L43–L46 Google Scholar
Holweger, H & Müller, EA 1974 Solar Phys. 39 19–30 Google Scholar
Withbroe, GL 1971 Nat. Bur. Stand. (U.S.) Spec. Publ. 353 127–148 Google Scholar