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Kinematics of Nearby FV Stars

Published online by Cambridge University Press:  04 August 2017

W.L.H. Shuter  and
W. N. Stocker
W.L.H. Shuter
Affiliation:
University of British Columbia
W. N. Stocker
Affiliation:
University of British Columbia

Extract

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The line-of-sight velocity field has been determined for all 80 FV stars within 15 degrees of the North Galactic Pole (NGP) with measured and constant velocities, and measured distances, from the catalogs of Hill et al. (1976, 1982). These data are a subset of the data used in a determination of Kz by Bahcall (1984). Procedures were as described by Goulet and Shuter (1984). The velocity field is depicted in Figure 1, and the magnitude of the velocity residuals is plotted in Figure 2.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 37
Copyright
Copyright © Reidel 1987 

References

Bahcall, J.N.: 1984, Astrophys. J., 287, p. 926.Google Scholar
Goulet, T., and Shuter, W.L.H.: 1984, in “Local Interstellar Medium”, eds. Kondo, Y. Bruhweiler, F.C. and Savage, B.D. (NASA), p. 319.Google Scholar
Hill, G. et al.: 1976, Mem. R. Astron. Soc., 82, p. 69.Google Scholar
Hill, G., Barnes, J.V., and Hilditch, R.W.: 1982, Publ. D.A.O., XVI, p. 111.Google Scholar