The Luminosity Function at the North and South Galactic Poles

Details The Luminosity Function at the North and South Galactic Poles The Luminosity Function at the North and South Galactic Poles

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..397k&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

Luminosity functions in the directions of the north and south galactic poles were derived by applying the Luyten mean absolute magnitude method to data from the galactic polar proper motion surveys by Luyten. The objective was to detect any differences between the luminosity functions at the north and south galactic poles. Both these luminosity functions were found to be consistent with the Luyten 1968 luminosity function and no significant difference between them was found.

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