The Chemical Evolution of Damped Lyman α Galaxies
1995; Springer Science+Business Media; Linguagem: Inglês
10.1007/978-3-540-49458-4_13
ISSN1611-6143
AutoresMax Pettini, David L. King, L. J. Smith, R. W. Hunstead,
Tópico(s)Astrophysical Phenomena and Observations
ResumoMeasurements of element abundances in damped Lyman α systems are providing new means to investigate the chemical evolution of galaxies, particularly at early times. We review progress in this area, concentrating on recent efforts to extend the range of existing surveys to both higher and lower redshifts.
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