Space Density Distribution of Late-Type Giants and Supergiants in the Solar Vicinity

Details Space Density Distribution of Late-Type Giants and Supergiants in the Solar Vicinity Space Density Distribution of Late-Type Giants and Supergiants in the Solar Vicinity

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..121i&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

Computer Science

Scientific paper

The star count data in the K band appearing in the Two-Micron Sky Survey are used to compute the space number density of the late giants and supergiants in the immediate solar vicinity and their effective height from the galactic plane. The space densities of early-type stars are also examined using the same data. The volume emissivity and surface brightness of the galactic disk at the solar distance are derived.

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