The internal kinematics of intermediate redshift galaxies
A dilemma is posed by studies of galaxy evolution at intermediate redshifts. If evolutionary effects are neglected, simple models predict number densities of faint galaxies which are 2—5x lower than observed at z ≅ 0.4. Yet the faint galaxy redshift distribution appears to be well modelled by the...
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| Format: | Others |
| Language: | English en |
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2018
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| Online Access: | https://dspace.library.uvic.ca//handle/1828/9740 |