Galaxy formation and evolution

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The deepest spectrum of the universe? Constraints on the Lyman continuum background at high redshift

HY-REDSHIFT UNIVERSE: GALAXY FORMATION AND EVOLUTION AT HIGH REDSHIFT 193 (1999) 262-266

Authors:

FR Marleau, AJ Bunker, JR Graham
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The mini-active galactic nucleus at the center of the elliptical galaxy NGC 4552 with Hubble Space Telescope

ASTROPHYSICAL JOURNAL 519:1 (1999) 117-133

Authors:

M Cappellari, A Renzini, L Greggio, SD Alighieri, LM Buson, D Burstein, F Bertola
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The peculiar motions of early-type galaxies in two distant regions -: V.: The Mg-σ relation, age and metallicity

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 303:4 (1999) 813-825

Authors:

M Colless, D Burstein, RL Davies, RK McMahan, RP Saglia, G Wegner
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The peculiar motions of early-type galaxies in two distant regions - II. The spectroscopic data

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 305:2 (1999) 259-296

Authors:

C Wegner, M Colless, RP Saglia, RK McMahan, RL Davies, D Burstein, G Baggley
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The spectral appearance of primeval galaxies

ASTR SOC P 200 (1999) 299-308

Authors:

B Guiderdoni, JEG Devriendt

Abstract:

The current and forthcoming observations of large samples of high-redshift galaxies selected according to various photometric and spectroscopic criteria can be interpreted in the context of galaxy formation, by means of models of evolving spectral energy distributions (SEDs). We hereafter present STARDUST which gives synthetic SEDs from the far UV to the submm wavelength range. These SEDs are designed to be implemented into semi-analytic models of galaxy formation.
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