Modeling multi-wavelength properties of high redshift galaxies

Details Modeling multi-wavelength properties of high redshift galaxies Modeling multi-wavelength properties of high redshift galaxies

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1111...48m&link_type=abstract

PROBING STELLAR POPULATIONS OUT TO THE DISTANT UNIVERSE: CEFALU 2008, Proceedings of the International Conference. AIP Conferen

Computer Science

2

Protogalaxies, Primordial Galaxies, Star Formation, Distances, Redshifts, Radial Velocities, Spatial Distribution Of Galaxies

Scientific paper

By comparing galaxy formation models within the ΛCDM cosmology with available data on high redshift galaxies, we show that small galaxies , with stellar masses <1011Msolar, are formed too early, are too passive since z~3 and too old at z = 0. This is due to an overproduction of small galaxies at high redshift, visible also as an excess of ZAB~27 V-dropouts. We discuss the consequences of this excess.

Affiliated with

Also associated with

No associations

Rating

Modeling multi-wavelength properties of high redshift galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Modeling multi-wavelength properties of high redshift galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling multi-wavelength properties of high redshift galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1109290