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Astrometric Tests of Galactic Evolution

Published online by Cambridge University Press:  07 August 2017

Gerard Gilmore*
Affiliation:
Institute of Astronomy, Madingley Rd, Cambridge, UK [email protected]

Extract

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There are many fundamental aspects of Galactic structure and evolution which can be studied best or exclusively with high quality three dimensional kinematics. Amongst these we note as examples determination of the orientation of the stellar velocity ellipsoid, and the detection of structure in velocity-position phase space. The first of these is the primary limitation at present to reliable and accurate measurement of the Galactic gravitational potential. The second is a critical test of current standard models of Galactic formation and evolution.

Type
2. Current and Future Needs for Very Accurate Astrometry
Copyright
Copyright © Kluwer 1995 

References

Cuddeford, P. & Amendt, P. (1992) MNRAS 256 166 Google Scholar
Eggen, O.J. (1987) in The Galaxy, eds Gilmore, G. & Carswell, R., p211 (Reidel)CrossRefGoogle Scholar
Fux, R. & Martinet, L. (1994), A&A, 287 L21 Google Scholar
Ibata, R., Gilmore, G., & Irwin, M. (1994) Nature 370 194 Google Scholar
Gilmore, G., Wyse, R.F.G., & Kuijken, K. (1989) ARAA 27 555 CrossRefGoogle Scholar
Kuijken, K. & Gilmore, G. (1989a) MNRAS 239 571 CrossRefGoogle Scholar
Kuijken, K. & Gilmore, G. (1989b) MNRAS 239 605 Google Scholar
Kuijken, K. & Gilmore, G. (1989c) MNRAS 239 651 Google Scholar
Kuijken, K. & Gilmore, G. (1991) Ap.J. 367 L9 CrossRefGoogle Scholar
Larsen, J.A. & Humphries, R. M. (1994) preprint Google Scholar
van der Marel, R.P. (1991), MNRAS, 248 515 CrossRefGoogle Scholar
Toth, G., & Ostriker, J. (1992) Ap.J. 389 5.Google Scholar