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Southern High-Velocity Stars

Published online by Cambridge University Press:  14 August 2015

H.J. Augensen  and
W. Buscombe
H.J. Augensen
Affiliation:
Northwestern University
W. Buscombe
Affiliation:
Northwestern University

Extract

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Using the model of the Galaxy presented by Eggen, Lynden-Bell and Sandage (1962), plane galactic orbits have been calculated for 800 southern high-velocity stars which possess parallax, proper motion, and radial velocity data. The stars with trigonometric parallaxes were selected from Buscombe and Morris (1958), supplemented by more recent spectroscopic data. Photometric parallaxes from infrared color indices were used for bright red giants studied by Eggen (1970), and for red dwarfs for which Rodgers and Eggen (1974) determined radial velocities.

Type
Poster Session
Information
Symposium - International Astronomical Union , Volume 80: The HR Diagram , 1978 , pp. 413 - 416
Copyright
Copyright © Reidel 1978 

References

Buscombe, W. and Morris, P.M. (1958). Mem. Mt. Stromlo Obs. 14.Google Scholar
Eggen, O.J. and Stokes, N.R. (1970). Astrophys. J. 161, 199.Google Scholar
Eggen, O.J., Lynden-Bell, D. and Sandage, A.R. (1962). Astrophys. J. 136, 748.CrossRefGoogle Scholar
Rodgers, A.W. and Eggen, O.J. (1974). Publ. Astron. Soc. Pacific 86, 428.CrossRefGoogle Scholar