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The Third Catalogue of Nearby Stars — Results and Conclusions
Published online by Cambridge University Press: 07 August 2017
Abstract
The nearby stars constitute the statistically most complete and therefore most representative sample of stars in our Galaxy. Only this sample allows a direct investigation of luminosity function and kinematics of low-mass stars.
A study of the Third Catalogue of Nearby Stars reveals a considerable increase — not only in quantity but also in quality — in our knowledge of the immediate solar neighbourhood, and reflects very nicely the progress achieved during the last decades — especially in astrometry and photometry. Expectations for the near future (HIPPARCOS) and desiderata for further astrometric and photometric work will be discussed.
- Type
- Ground-Based Optical Astrometry
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- Copyright © Kluwer
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