The Luminosity Function at High Galactic Latitudes

Details The Luminosity Function at High Galactic Latitudes The Luminosity Function at High Galactic Latitudes

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..427u&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

Scientific paper

Luminosity functions have been determined for stars at distances 100,
200 and 400 pc above the galactic plane and at 100 and 200 pc below the
galactic plane. With increasing distance from the plane the contribution
from Population II stars increases relative to Population I stars.

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