Volume 367, Number 1, February III 2001
|Page(s)||106 - 110|
|Published online||15 February 2001|
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.