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Systematic Spectroscopic Observations on Small Telescopes: Past and Future Research of Stellar Kinematics

Published online by Cambridge University Press:  12 April 2016

M.E. Sachkov ,
E.V. Glushkova  and
A.S. Rastorguev
M.E. Sachkov
Affiliation:
Institute of Astronomy, 48 Pyatnitskaya Str., Moscow 109017, Russia
E.V. Glushkova
Affiliation:
Sternberg Astronomical Institute, 13 Universitetsky Ave., Moscow 119899, Russia
A.S. Rastorguev
Affiliation:
Sternberg Astronomical Institute, 13 Universitetsky Ave., Moscow 119899, Russia

Abstract

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We have used a CORAVEL-type spectrometer on small telescopes (70-cm, Moscow observatory, Russia; 60- and 100-cm, Simeiz observatory, Crimea, Ukraine and some others) for systematic observations of northern sky stars, since 1987 (Rastorguev & Glushkova, 1997; Gorynya et al., 1998). The typical accuracy of a single measurement is about 0.5 km/s. The limiting magnitude is 14 in V-band. The young Galaxy disk population, metal-poor stars and Kaptein selected areas are the important parts of our program. In this paper we present new results on galactic kinematics and our future program.

Type
VII. Science With Small Telescopes
Information
International Astronomical Union Colloquium , Volume 183: Small-Telescope Astronomy on Global Scales , 2001 , pp. 327 - 328
Copyright
Copyright © Astronomical Society of the Pacific 2001

References

ESA, 1997, The Hipparcos and Tycho Catalogues, SP-1200.Google Scholar
Rastorguev, A.S., Glushkova, E.V. 1997, Astronomy Letters, V.23, P.1.Google Scholar
Gorynya, N.A., Samus, N.N., Sachkov, M.E., Rastorguev, A.S., Glushkova, E.V., and Antipin, S.V. 1998, Astronomy Letters, V.24, P. 815.Google Scholar