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Observations of Faint Globular Clusters

Published online by Cambridge University Press:  12 April 2016

L. Rosino  and
G. Pinto

Extract

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The present communication reports some results of observations made at Asiago on three faint globular clusters discovered on Palomar Sky Survey plates (Abell 1955).

Palomar 2 (4h43.m1, + 31 °23’, 1950; l= 170°, b= -9°). This cluster was studied some years ago by McCarthy and Treanor (1964) on infrared plates taken with the Schmidt telescope of the Vatican Observatory. After an extensive discussion the authors concluded that the object was either a peculiar globular cluster at an estimated distance of 63 kpc or an old galactic cluster at a distance of the order of 16 kpc.

Type
Part I / General Problems of Variables in Population II Systems
Information
International Astronomical Union Colloquium , Volume 21: Variable Stars in Globular Clusters and in Related Systems , August 1973 , pp. 21 - 25
Copyright
Copyright © Reidel 1973

References

Abell, G. O.: 1955, Publ. Astron. Soc. Pacific 67, 258.Google Scholar
Burbidge, E. M. and Sandage, A.: 1958, Astrophys. J. 127, 527.CrossRefGoogle Scholar
Kinman, T. D. and Rosino, L.: 1962, Publ. Astron. Soc. Pacific 74, 499.Google Scholar
Mannino, G.: 1956, Pubbl. Oss. astr. Univ. Bologna VI, 17.Google Scholar
McCarthy, M. F. and Treanor, P. J.: 1964, Ric. astr. Specola Vatic. 6, 24.Google Scholar
Pietra, S.: 1956, Pubbl. Oss. astr. Univ. Bologna VI, 16.Google Scholar
Rosino, L.: 1951, Pubbl. Oss. astr. Univ. Bologna VI, 15.Google Scholar
Rosino, L.: 1957, Contr. Oss.astrofis. Univ. Padova No.85.Google Scholar