Further evidence concerning the local density of red dwarfs

Details Further evidence concerning the local density of red dwarfs Further evidence concerning the local density of red dwarfs

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...204..113w&link_type=abstract

Astrophysical Journal, vol. 204, Feb. 15, 1976, pt. 1, p. 113-115.

Astronomy and Astrophysics

Astrophysics

24

Astronomical Photometry, Dwarf Stars, Star Distribution, Stellar Luminosity, Electrophotometry, Stellar Spectra

Scientific paper

Recent evidence has suggested the existence of a large number of red dwarfs, highly concentrated to the galactic plane, in the solar neighborhood. These results are reexamined using photoelectrically determined B-V and (R-I)W colors for a sample of stars near the North Galactic Pole. Preliminary analysis of the data indicates that the density of the reddest stars is not nearly as great as was previously reported.

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