Chemical Evolution from Zero to High Redshift: Proceedings of the ESO Workshop Held at Garching, Germany, 14–16 October 1998 (ESO Astrophysics Symposia)

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9783662216972: Chemical Evolution from Zero to High Redshift: Proceedings of the ESO Workshop Held at Garching, Germany, 14–16 October 1998 (ESO Astrophysics Symposia)

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

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From the Back Cover :

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.

Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.

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Description du livre Springer. Paperback. État : New. Paperback. 314 pages. Dimensions: 9.0in. x 6.0in. x 0.8in.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 ZO This item ships from multiple locations. Your book may arrive from Roseburg,OR, La Vergne,TN. Paperback. N° de réf. du libraire 9783662216972

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Description du livre Springer-Verlag Berlin and Heidelberg GmbH Co. KG, Germany, 2014. Paperback. État : New. Language: English . Brand New Book ***** Print on Demand *****.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 Softcover reprint of the original 1st ed. 1999. N° de réf. du libraire AAV9783662216972

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