Chemical Evolution from Zero to High Redshift: Proceedings of the ESO Workshop Held at Garching, Germany, 14-16 October, 1998
Jeremy R. Walsh, Michael R. Rosa
Springer, Jan 1, 1999 - Science - 312 pages
The observational and interpretive tools for the study of chemical evolution are starting to be mature enough that they can be applied with some confidence to extra-galactic systems and integrated populations at increasingly high redshift. This book is devoted to the study of the interplay between different methods of measuring chemical abundances with astrophysical models. Studies of chemical abundances and evolution from stars, inter-stellar medium and local group galaxies at zero redshift to distant galaxies, clusters of galaxies and inter-galactic medium at high redshift are presented. There are also synopses on progress in instrumentation for abundance determination.
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Chemical Abundances of Local Unevolved Stars
Nebular Abundances from Recombination Lines
Constraints on the Nature of Interstellar Dust
8 other sections not shown
absorption lines abundance gradients abundance ratios accretion Astronomy baryons bulge chemical abundances chemical evolution clouds cluster column density continuum correlation derived detected detector DLAs dust dwarf galaxies Edmunds element abundances elliptical enrichment Fe/H fraction function Galactic bulge Galactic disk Galactic halo Garching Garnett gas-phase halo heavy elements high redshift HII regions images interstellar ionization iron irregular galaxies Izotov Kennicutt luminosity mass massive stars Matteucci measured metal-poor metallicity MNRAS models nebula Nomoto nucleosynthesis Observatory observed optical oxygen abundance Pagel parameters Peimbert Pettini planetary nebulae predicted quasar radial range redshift Renzini sample Skillman solar Songaila spectra spectrograph spectroscopy spectrum spiral galaxies star formation star formation rate star-forming starburst starburst galaxies Steidel stellar population studies supergiants supernova telescopes temperature Thuan Torres-Peimbert values wavelength Woosley X-ray yields