9781402012891 - The IGM/Galaxy Connection: The Distribution of Baryons at z=0: 281 (Astrophysics and Space Science Library, 281) (19 resultados)

Condición: Good. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,900grams, ISBN:9781402012891.

Condición: New. In.

Condición: New.

Condición: New.

Condición: New. This is a Brand-new US Edition. This Item may be shipped from US or any other country as we have multiple locations worldwide.

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Condición: New. pp. 374.

Condición: New. pp. 374 Illus.

Condición: New. 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. . . . .

Condición: New. pp. 374.

Hardcover. Condición: Brand New. 1st edition. 368 pages. 10.00x6.50x0.75 inches. In Stock.

Condición: New. 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. . . . . Books ship from the US and Ireland.

Buch. Condición: Neu. Druck auf Anfrage Neuware - Printed after ordering - 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.

Condición: As New. Unread book in perfect condition.

Hardcover. Condición: Like New. Like New. book.

Condición: As New. Unread book in perfect condition.

Gebunden. Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. 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 fo.

Buch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -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.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 372 pp. Englisch.

Buch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -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. 372 pp. Englisch.