Chemical Evolution from Zero to High Redshift - Proceedings of the ESO Workshop Held at Garching, Germany, 14-16 October 1998 (Paperback, Softcover reprint of the original 1st ed. 1999)

With the new era of 8-10 m telescopes the power to spectroscopically examine the light of fainter and more distant targets has taken a 'photon' leap. It is now becoming routinely possible to obtain high signal-to-noise spectra of very distant objects and to attempt the determination of their abundances. The motivation for a workshop on this topic could be summarized thus: Do we understand enough about chemical abundances at zero redshift to trust any conclusions on chem- ical evolution at high redshift? Given our observational background in gaseous nebulae, we thought at first in terms of a workshop largcly devoted to the inter- stellar medium. However, we were encouraged by Jacqueline Bergeron and Alvio Renzini to pitch the theme much wider. The members of the Scientific Organiz- ing Committee (Francoise Combes, Don Garnett, Guinevere Kauffmann, Claus Leitherer, Danny Lennon, Max Pettini, Peter Shaver, Elena Terlevich and David Tytler), under the chair of John Mathis, made sure that we kept the conference broad in scope. We thank them for their encouragement and advice. Informally the working title for the conference thus became "High and low Z from low to high z" (or Z@O

General

Imprint:	Springer-Verlag
Country of origin:	Germany
Series:	ESO Astrophysics Symposia
Release date:	April 2014
First published:	1999
Editors:	Jeremy Walsh • Michael R. Rosa
Dimensions:	235 x 155 x 18mm (L x W x T)
Format:	Paperback
Pages:	314
Edition:	Softcover reprint of the original 1st ed. 1999
ISBN-13:	978-3-662-21697-2
Categories:	Books > Science & Mathematics > Astronomy, space & time > General
LSN:	3-662-21697-3
Barcode:	9783662216972

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