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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

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