
doi: 10.5282/edoc.36328
Diese Arbeit präsentiert eine Studie über die Kinematik und die chemische Häufigkeitsverteilung massereicher sternbildender Galaxien (SFGs) während der ersten 1.5 Milliarden Jahre nach dem Urknall bei Rotverschiebungen von 4
This thesis presents a study of the kinematics and chemical abundance distributions of massive star-forming galaxies (SFGs) during the 1.5 billion years after the Big Bang at redshifts 4
500, FOS: Physical sciences, 530, High-redshift galaxies, Galaxy kinematics, Galaxy dynamics, Astronomy data analysis, Astronomy data modelling, Galaxy abundances
500, FOS: Physical sciences, 530, High-redshift galaxies, Galaxy kinematics, Galaxy dynamics, Astronomy data analysis, Astronomy data modelling, Galaxy abundances
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