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Kinematical and chemical evolution of the Galactic disk

Published online by Cambridge University Press:  04 August 2017

Cedric G. Lacey  and
S. Michael Fall
Cedric G. Lacey
Affiliation:
Institute of Astronomy, Cambridge, England
S. Michael Fall
Affiliation:
Institute of Astronomy, Cambridge, England

Extract

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We have calculated models for the kinematical and chemical evolution of the Galactic disk that include the infall of metal-free gas and the stochastic acceleration of disk stars. Our models are similar in some respects to those of Chiosi (1980) and Vader & de Jong (1981), but the results are compared with a greater variety of observational data. A complete description of this work will appear shortly in Monthly Notices of the Royal Astronomical Society.

Type
PART III: Dynamics and Evolution
Information
Symposium - International Astronomical Union , Volume 106: The Milky Way Galaxy , 1985 , pp. 597 - 600
Copyright
Copyright © Reidel 1985 

References

Chiosi, C.: 1980, Astron. Astrophys. 83, p. 206 Google Scholar
Schmidt, M.: 1959, Astrophys. J. 129, p. 243 CrossRefGoogle Scholar
Vader, J.P., and de Jong, T.: 1981, Astron. Astrophys. 100, p. 124 Google Scholar
Wielen, R.: 1977, Astron. Astrophys. 60, p. 263 Google Scholar