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Proper Motions Of 47 TUC And NGC 362 Relative To The Small Magellanic Cloud

Published online by Cambridge University Press:  03 August 2017

H.-J. Tucholke*
Affiliation:
Astronomisches Institut der Universität Münster, Wilhelm-Klemm-Str. 10, D-4400 Münster, F.R.G.

Abstract

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The proper motions of the galactic globular clusters 47 Tuc and NGC 362 are currently being measured relative to the background of the Small Magellanic Cloud. This paper reports on the reduction routines developed so far for the simultaneous computation of several thousands of stellar proper motions. A preliminary result for NGC 362 is given.

Type
Part II: Current Research
Copyright
Copyright © Kluwer 1988 

References

Bolte, M. (1987). Astrophys. J. 315, 469.Google Scholar
Brosche, P.; Geffert, M.; Klemola, A.R.; Ninkovic, S. (1985). Astron. J. 90, 2033.Google Scholar
Lin, D.N.C.; Lynden-Bell, D. (1982). Mon. Not. R. Astron. Soc. 198, 707.Google Scholar
Russell, J.L. (1986). In IAU Symposium 109, Astrometric Techniques, eds. Eichhorn, H. and Leacock, R.J. (Reidel, Dordrecht), p. 697.CrossRefGoogle Scholar
Tucholke, H.-J. (1983). , Astron. Inst. Univ. Münster.Google Scholar
Tucholke, H.-J.; Brosche, P.; Geffert, M. (1987). In IAU Symposium 126, Globular Cluster Systems in Galaxies, eds. Grindlay, J.E. and Davis Philip, A.G., in press.Google Scholar