Kinematical Properties of the Spectral Group of Nearby Dwarfs

Details Kinematical Properties of the Spectral Group of Nearby Dwarfs Kinematical Properties of the Spectral Group of Nearby Dwarfs

Dec 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jkas...14...73l&link_type=abstract

Journal of the Korean Astronomical Society, vol. 14, no. 2, p. 73-78

Astronomy and Astrophysics

Astronomy

1

Scientific paper

On the basis of the recently available data, we have analysed the kinematical properties nearby dwarfs, which are grouped by their spectral types and derived their ages from the kinmatical properties. The discontinuities in the kinematical properties are found around late F stars, which appear to be caused mainly by the fact that the spectral groups earlier than late F are rather homogeneous in age while the later ones are mixed by two different age groups.

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