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Observational Constraints for the Chemical Evolution of the Solar Neighbourhood

Published online by Cambridge University Press:  12 April 2016

M. Grenon
M. Grenon*
Affiliation:
Observatoire de Genève

Extract

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The basic material for this preliminary investigation is formed of the Northern stare of Gliese’s catalogue, completely measured down to the K5 spectral type in the Geneva system. The physical properties and new spatial velocities are derived and, after removal of non members of the local sphere, 230 stars can be used here.

Type
Part III: The Chemical Properties of the Disc and the Halo in our Galaxy
Information
International Astronomical Union Colloquium , Volume 45: Chemical and Dynamical Evolution of our Galaxy , September 1977 , pp. 169 - 172
Copyright
Copyright © Geneva Observatory 1977

References

Grenon, M. 1975, David Dunlap Obs. Report, 9, 413 Google Scholar
Larson, R.B. 1975, M.N.R.A.S. 173, 671 Google Scholar
Mayor, M. 1977, Private communicationGoogle Scholar
Pagel, B.E.J., Patchett, B.E. 1975, M.N.R.A.S. 172, 13 Google Scholar
Peimbert, M., Torres-Peimtbert, S. 1976, Ap. J. 203, 581 CrossRefGoogle Scholar
Woolley, R. 1968, Galactic Astronomy, Chiu, and Muriel, Ed., 95 Google Scholar