Other
Scientific paper
Dec 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997apl%26c..36..367l&link_type=abstract
Astrophysical Letters and Communications, Vol. 36, Nos. 1 - 6, p. 367 - 374
Other
Disk Galaxies: Interstellar Absorption, Galaxy Counts: Interstellar Absorption, Cosmology: Galaxy Counts
Scientific paper
Assuming that, during the evolution of disk galaxies, interstellar dust is continually produced and added to the interstellar medium, the authors model the opacity of galactic disks as a function of redshift. This opacity effect will affect galaxy number counts, producing an excess at faint magnitudes (compared to no-evolution models). Magnitude limited surveys will show more galaxies at large redshifts than otherwise expected.
Leroy Peter
Portilla Miguel
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