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Comparison of Secular Parallaxes Determined from Proper Motions of Stars Relative to Galaxies at the Pulkovo and Lick Observatories

Published online by Cambridge University Press:  14 August 2015

N. V. Fatchikhin
N. V. Fatchikhin*
Affiliation:
Pulkovo Observatory, U.S.S.R.

Extract

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The secular parallaxes, determined by Klemola and Vasilevskis from proper motions of stars relative to galaxies (Klemola and Vasilevskis, 1971), were interpolated in latitude for each area of the Pulkovo Catalogue (Fatchikhin, 1974). Then the mean values were grouped in three zones of galactic latitude (b) and the data obtained at the Lick Observatory (L) were compared with our data (P) (Fatchikhin, 1972, 1973). The results are given in the Table I.

Type
Session E: Proper Motions and Galactic Problems
Information
Symposium - International Astronomical Union , Volume 61: New Problems in Astrometry , 1974 , pp. 205 - 206
Copyright
Copyright © Reidel 1974 

References

Fatchikhin, N. V.: 1974, ‘Catalogue of 14600 Stars’, Trudy Pulkovo Obs. 81, in press.Google Scholar
Fatchikhin, N. V.: 1972, Astron. Circ. Acad. Sci. U.S.S.R. , No. 668.Google Scholar
Fatchikhin, N. V.: 1973, Astron. Zh. 50, 2.Google Scholar
Klemola, A. R. and Vasilevskis, S.: 1971, Publ. Lick Obs. 22, 111.Google Scholar