Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.260..610a&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 260, no. 3, p. 610-616.
Astronomy and Astrophysics
Astronomy
22
Dark Matter, Galactic Halos, Galactic Mass, Spiral Galaxies, Galactic Clusters, Galactic Evolution, Luminosity, Mass To Light Ratios
Scientific paper
We derive the mass function of spiral galaxy haloes using the luminosity function and the inferred variation in mass-to-light ratio with spiral galaxy luminosity. We show that the resulting mass function is consistent with hierarchical clustering models of galaxy formation. This contrasts with previous results based on the assumption of a constant mass-to-light ratio for all spirals, which predict too many low-luminosity galaxies. By reversing the argument, we show that, if spirals form through hierarchical clustering, then the observed luminosity function requires an increase in the dark matter fraction with decreasing luminosity.
Ashman Keith M.
Persic Massimo
Salucci Paolo
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