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Motions of Near-Polar K-Giants Along the Z-Coordinate

Published online by Cambridge University Press:  30 March 2016

A. N. Balakirev
A. N. Balakirev*
Affiliation:
Sternberg Astronomical Institute Moscow UniversityMoscow, U.S.S.R.

Extract

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The motion of G8-K5 III, IV stars near galactic poles (|b|>60°) was investigated. The main attention was paid to motion in the z-direction. The spectral types, visual magnitudes, colors and radial velocities (vr) were taken mainly from Schild (1973), Heard (1956), Blanco et al (1968) and Wilson (1953). To reduce the values vr by Heard to those by Wilson, the correction of -1 km/sec was made. The stars with variable vr and spectroscopic binaries were excluded from the investigation.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 4 , Issue 2: Highlights of Astronomy. As presented at the XVIth General Assembly of the IAU, 1976 (Part II) , 1977 , pp. 83 - 86
Copyright
Copyright © Reidel 1977

References

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The full text of this paper is published in Astron.Zhur. SSSR 1976, 53., 1 (see Soviet Astronomy 1976, 20, 64).Google Scholar