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The Population of Open Clusters in the Nearest kpc from the Sun

Published online by Cambridge University Press:  01 September 2007

S. Röser ,
N. V. Kharchenko ,
A. E. Piskunov ,
E. Schilbach  and
R.-D. Scholz
S. Röser
Affiliation:
Astronomisches Rechen-Institut, Moenchhofstr. 12-14, 69120 Heidelberg, Germany email: roeser@ari.uni-heidelberg.de
N. V. Kharchenko
Affiliation:
Astronomisches Rechen-Institut, Moenchhofstr. 12-14, 69120 Heidelberg, Germany email: roeser@ari.uni-heidelberg.de Main Astronomical Observatory, Kiev, Ukraine Astrophysikalisches Institut Potsdam, Potsdam, Germany
A. E. Piskunov
Affiliation:
Astronomisches Rechen-Institut, Moenchhofstr. 12-14, 69120 Heidelberg, Germany email: roeser@ari.uni-heidelberg.de Institute of Astronomy of the Russian Acad. Sci., Moscow, Russia Astrophysikalisches Institut Potsdam, Potsdam, Germany
E. Schilbach
Affiliation:
Astronomisches Rechen-Institut, Moenchhofstr. 12-14, 69120 Heidelberg, Germany email: roeser@ari.uni-heidelberg.de
R.-D. Scholz
Affiliation:
Astrophysikalisches Institut Potsdam, Potsdam, Germany
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Abstract

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We present a volume-limited sample (d < 850 pc) of open clusters in the Galaxy identified from our studies on galactic open clusters based on data from the all-sky catalogue ASCC-2.5 with absolute proper motions and B, V magnitudes of 2.5 million stars. The astrophysical properties of this sample are discussed.

Keywords

open clusters and associations: generalGalaxy: kinematics and dynamicstechniques: photometricastrometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 3 , Symposium S246: Dynamical Evolution of Dense Stellar Systems , September 2007 , pp. 115 - 116
Copyright
Copyright © International Astronomical Union 2008

References

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Kharchenko, N. V. 2001, Kinematics and Physics of Celestial Bodies 17, 409 (ASCC-2.5, Cat. I/280A)Google Scholar
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