Hostname: page-component-848d4c4894-wzw2p Total loading time: 0 Render date: 2024-05-01T06:48:04.829Z Has data issue: false hasContentIssue false
  • English
  • Français

The Chemical Evolution of the Galactic Disc, Investigated by Abundance Analysis of F Stars: A Progress Report

Published online by Cambridge University Press:  04 August 2017

B. Edvardsson ,
P. E. Nissen ,
B. Gustafsson  and
J. Andersen
B. Edvardsson
Affiliation:
Uppsala Astronomical Observatory
P. E. Nissen
Affiliation:
Astronomical Institute, Aarhus
B. Gustafsson
Affiliation:
Stockholm Observatory
J. Andersen
Affiliation:
Astronomical Observatory, Brorfelde

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.

An extensive project for the investigation of abundances, especially of light elements, in F-type stars is described and some preliminary results are given.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 575 - 579
Copyright
Copyright © Reidel 1985 

References

Blackwell, D.E. and Shallis, M.J. 1977, Mon. Not. R. astr. Soc. 180, 177 Google Scholar
Dravins, D., Lindegren, L. and Nordlund, Å, 1981, Astron. Astrophys. 96, 345 Google Scholar
Gehren, T. 1981, Astron. Astrophys. 100, 97 Google Scholar
Gustafsson, B., Bell, R.A., Eriksson, K. and Nordlund, Å. 1975, Astron. Astrophys. 42, 407 Google Scholar
Nissen, P.E. and Gustafsson, B. 1978, Astronomical Papers dedicated to Bengt Strömgren, Eds. Reiz, A., Andersen, T., (Copenhagen University Observatory), p. 43 Google Scholar
Saxner, M. 1984, , Uppsala University; to be submitted to Astron. Astrophys. Google Scholar