Physics
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf...81b&link_type=abstract
The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ
Physics
1
Scientific paper
The extensive proper-motion-star spectral classification programs of the late G. P. Kuiper and of S.-G. Lee, which have provided spectral types for many hundreds of stars for which such information is presently not available, are discussed. Kuiper's work concentrated on the then-known northern hemisphere proper-motion stars of μ > 0arcsec.30 and on the southern (down to δ = -50°) objects of μ ≥ 0arcsec.50; Lee's work deals with the Lowell Observatory northern-hemisphere stars (≥0arcsec.26) brighter than mpg = 13.5.
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