The bulge luminosity functions in the MSX infrared bands
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain
2 Radio Astronomy Laboratory, 601 Campbell Hall, University of California, Berkeley, CA 94720, USA
Corresponding author: M. López-Corredoira, firstname.lastname@example.org
Accepted: 30 November 2000
We use an inversion technique to derive the luminosity functions of the Galactic bulge from point source counts extracted from the Midcourse Space Experiment's Point Source Catalog (version 1.2).
Key words: Galaxy: stellar content / Galaxy: structure / infrared: stars
© ESO, 2001