The Effect of Changes in the Luminosity Function on Problems in Galactic Structure

Details The Effect of Changes in the Luminosity Function on Problems in Galactic Structure The Effect of Changes in the Luminosity Function on Problems in Galactic Structure

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..229a&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

4

Scientific paper

The author considers the Bahcall-Soneira Galaxy model and the
Miller-Scalo initial mass function and investigates effects depending on
the choice of stellar luminosity functions. The cases of Luyten's and
Wielen's luminosity functions are discussed.

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