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Galactic Structure with GSC-II Material

The North Galactic Pole and the Stock-2 cluster regions

Published online by Cambridge University Press:  25 May 2016

A. Spagna ,
M.G. Lattanzi ,
G. Massone ,
B.J. McLean  and
B.M. Lasker
A. Spagna
Affiliation:
Osservatorio Astron. di Torino
M.G. Lattanzi
Affiliation:
Osservatorio Astron. di Torino
G. Massone
Affiliation:
Osservatorio Astron. di Torino
B.J. McLean
Affiliation:
Space Telescope Science Institute
B.M. Lasker
Affiliation:
Space Telescope Science Institute

Extract

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Faint surveys of accurate colors and proper motions are fundamental for studying the physical and kinematical properties of the stellar populations in the Galaxy. A program designed to address such issues has been initiated on selected fields utilizing prototype material from the GSC-II project (see McLean et al. in this volume, p. 431). Photographic photometry V, B–V, V–Rc, is derived down to V = 18.5 with a precision of about 0.1 mag, together with absolute proper motions to σμ ≃ 3 mas/yr.

Type
Part 4. Galactic Structure
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 228 - 230
Copyright
Copyright © Kluwer 1998 

References

Bahcall, J. N., Casertano, S., and Ratnatunga, K. U. 1987. Astrophys. J., 320, 515.Google Scholar
Bienaymé, O., Robin, A.C. and Crézé, M., 1987. Astron. Astrophys., 180, 94.Google Scholar
Krzeminsky, W. and Serkowski, K., 1967. Astron. J., 147, 988.Google Scholar
Ratnatunga, K. U., Bahcall, J. N., and Casertano, S. 1989. Astrophys. J., 339, 106.Google Scholar
Robin, A.C. and Crézé, M., 1986. Astron. Astrophys., 157, 71.Google Scholar
Spagna, A., et al. 1996. Astron. Astrophys, 311, 758.Google Scholar