The IGM/galaxy Connection. The Distribution of Baryons at Z=0.

. Ed(s): Rosenberg, Jessica L.; Putman, Mary E.

ISBN 10: 1402012896 / ISBN 13: 9781402012891

Published by Kluwer Academic Publishers, 2003

About this Item

Examines the census of baryons in the local universe as a function of the states in which they reside and how they evolve with redshift. This book characterizes the halos around galaxies and discusses the relics of the galaxy formation process from a theoretical perspective, and by observational and theoretical analysis of the feedback mechanisms. Editor(s): Rosenberg, Jessica L.; Putman, Mary E. Series: Astrophysics and Space Science Library. Num Pages: 367 pages, biography. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational; (UP) Postgraduate, Research & Scholarly; (UU) Undergraduate. Dimension: 235 x 155 x 22. Weight in Grams: 700. . 2003. Hardback. . . . .

Seller Inventory # V9781402012891

Bibliographic Details

• Title: The IGM/galaxy Connection. The Distribution of Baryons at Z=0.
• Publisher: Kluwer Academic Publishers
• Publication Date: 2003
• Language: English
• ISBN 10: 1402012896
• ISBN 13: 9781402012891
• Binding: Hardcover
• Condition: New

About this title

Synopsis

This volume contains the proceedings of the meeting entitled, "The IGM/Galaxy Connection: The Distribution of Baryons at z = 0. " The meeting was held August 8 -10 at the National Center for Atmospheric Research (NCAR) located in Boulder, Colorado on the foothills of the Rocky Mountains (see conference photo). We organized this meeting because we felt it was time to address the link between galaxies and the intergalactic medium at low redshift. In this vein, we posed several questions to the conference participants: Where are the baryons in the local universe and in what phase do they reside? What signatures of galaxy evolution have been imprinted on the IGM? What percentage of intergalactic gas is left from the galaxy formation process? What does the distribution of baryons at z = 0 tell us about the early universe? The conference was an overwhelming success with lots of friendly interaction and discussion among the participants. At lunch we were treated to splendid views from the NCAR terrace and discussions rang­ ing from the importance of the LSR, GSR, and LGSR velocity frames to how long the desserts would last with 90 astronomers and the hot Boul­ der sun. From an inventory of the baryons, to the associations between galaxies and Lya absorbers, to the mechanisms by which galaxies obtain and lose gas, the conference covered many topics. The results of these endeavors are contained in these pages and eloquently summarized by Chris Impey.