Distributions and Motions of Nearby Stars defined by Objective Prism Surveys and HIPPARCOS

Details Distributions and Motions of Nearby Stars defined by Objective Prism Surveys and HIPPARCOS Distributions and Motions of Nearby Stars defined by Objective Prism Surveys and HIPPARCOS

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..549h&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 549-550

Physics

Scientific paper

Material from objective prism spectral classification work is used to determine the space density distribution of nearby common stars to the limits of objective prism spectral surveys and, more specifically, to extend the knowledge of the local densities of specific spectral types from a radius of 25 pc from the Sun, as limited in the Catalogue of Nearby Stars by Gliese, to 50 pc or more. Future plans for the application of these results to studies of the kinematic and dynamical properties of the stars in the solar neighbourhood as a function of their physical properties and ages are described.

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