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Evolving Universe : Selected Topics on Large-Scale Structure and on the Prope...
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eBay-Artikelnr.:176653686683
Artikelmerkmale
- Artikelzustand
- Book Title
- Evolving Universe : Selected Topics on Large-Scale Structure and
- ISBN
- 9780792350743
Über dieses Produkt
Product Identifiers
Publisher
Springer Netherlands
ISBN-10
079235074X
ISBN-13
9780792350743
eBay Product ID (ePID)
23038810671
Product Key Features
Number of Pages
VIII, 433 Pages
Language
English
Publication Name
Evolving Universe : Selected Topics on Large-Scale Structure and on the Properties of Galaxies Based upon, in Part, Contributions to the Ringberg Workshop on Large-Scale Structure, Ringberg Castle, 23-28 September, 1996
Subject
Physics / Astrophysics, Astronomy, Gravity
Publication Year
1998
Type
Textbook
Subject Area
Science
Series
Astrophysics and Space Science Library
Format
Hardcover
Dimensions
Item Weight
62.1 Oz
Item Length
9.6 in
Item Width
6.7 in
Additional Product Features
Intended Audience
Scholarly & Professional
LCCN
98-020102
Dewey Edition
21
TitleLeading
The
Series Volume Number
231
Number of Volumes
1 vol.
Illustrated
Yes
Dewey Decimal
523.1/1
Table Of Content
and Preface.- The Nearby Universe.- Large-Scale Structure and the Nearby Universe.- The Galaxy Luminosity Function at Zero Redshift: Constraints on Galaxy Formation.- CfA Surveys and Their Extensions.- The Spatial Distribution of Emission-Line Galaxies.- Properties of Galaxies In and Around Voids.- Large-Scale Flows from the Mark III Tully-Fisher Data.- The Luminosity Function and the Mean Galaxy Density from the ESO Slice Project (ESP).- The Münster Redshift Project.- The Las Campanas Redshift Survey.- Geometry and Large-Scale Power in the Las Campanas Redshift Survey.- The Las Campanas Redshift Survey Results: The Redshift-Space Autocorrelation Function.- The Las Campanas Redshift Survey Results:.- The Moderate Redshift Universe.- The CNOC Cluster Survey.- Results from The Norris Survey of the Corona Borealis Supercluster.- Clustering at z > 0.8.- A Massive Cluster of Galaxies at z.- Redshift Distortions.- Linear Redshift Distortions: A Review.- Future Surveys.- The Sloan Digital Sky Survey.- Absorption-Line Based Studies.- The Large-Scale Distribution of Baryons at High Redshift.- Simulations of the Large-Scale Structure Formation & The Evolution of the Lyman-a Forest: Comparison with Observations.- Probing Small-and Large-Scale Structure at High Redshift with the TPCF of CD/ Absorption Lines.- Hubble Deep Field Analyses.- Lines and Lenses in The Hubble Deep Field.- Interpreting High-Redshift Galaxies in the HDF.- Theory and Theoretical Analyses of Observational Data.- The 3-Point Correlation Function of the Cosmic Matter Distribution.- Analytic Approximations to Galaxy Clustering.- High Redshift Objects in the Cosmic String Model.- Analyzing Redshift Surveys to Measure The Power Spectrum on Large Scales.- Constraints on the Large-Scale Gas Distribution from CMB--X-Ray Correlations.- Estimates for the Luminosity Function and Selection Function of Redshift Surveys.- The Virgo Consortium: The Formation and Evolution of Galaxy Clusters.- Toward High-Precision Measures of Large-Scale Structure.- Miscellaneous.- Search for Primeval Galaxies with CADIS.- Group Photograph of the Ringberg Workshop Participants.
Synopsis
1. The Workshop and this Tome In the excellent bucolic setting of SchloB Ringberg in Upper Bavaria, over 50 scientists assembled during the week of 23-28 September 1996 to discuss recent results, both theoretical and observational in nature, on the large- scale structure of the Universe. Such a topic is perhaps nowadays far too encompassing, and is essentially all of what we used to call "observational cosmology. " The original philosophy of the organization of this meeting was deliber- ated aimed at the younger community and their contributions. As a conse- quence, the content of the presentations was refreshingly new, as it should be. In spite of the deficiences caused by the lack of certain key researchers in this field, for one reason or another, the final result was rewarding to all. Although the conference was held in Fall 1996, the contributions contained herein were submitted as late as Spring 1998, thus the content maintains some degree of trendiness. Originally the current volume was to be a "proceedings. " This refers to the usual archival tome that fills one's shelf and is rarely consulted, except to see the canonical group photo, which by the way, we also have. Nevertheless, I wanted something more than that. Although the field is rapidly changing, with so-called facts in a state ofconstant volubility, now is a good time for reflection prior to the commencement ofthe Sloan Survey, presumably the definitive large-scale program of low- to moderate-redshift galaxies in our lifetime., 1. The Workshop and this Tome In the excellent bucolic setting of SchloB Ringberg in Upper Bavaria, over 50 scientists assembled during the week of 23-28 September 1996 to discuss recent results, both theoretical and observational in nature, on the large scale structure of the Universe. Such a topic is perhaps nowadays far too encompassing, and is essentially all of what we used to call "observational cosmology. " The original philosophy of the organization of this meeting was deliber ated aimed at the younger community and their contributions. As a conse quence, the content of the presentations was refreshingly new, as it should be. In spite of the deficiences caused by the lack of certain key researchers in this field, for one reason or another, the final result was rewarding to all. Although the conference was held in Fall 1996, the contributions contained herein were submitted as late as Spring 1998, thus the content maintains some degree of trendiness. Originally the current volume was to be a "proceedings. " This refers to the usual archival tome that fills one's shelf and is rarely consulted, except to see the canonical group photo, which by the way, we also have. Nevertheless, I wanted something more than that. Although the field is rapidly changing, with so-called facts in a state ofconstant volubility, now is a good time for reflection prior to the commencement ofthe Sloan Survey, presumably the definitive large-scale program of low- to moderate-redshift galaxies in our lifetime., The Evolving Universe is a compendium of topics on and related to the large-scale structure of the Universe. These include galaxy luminosity functions and their dependence upon environment and galaxy type; clustering of galaxies; evolution of the clustering of galaxies; rich clusters of galaxies; superclusters of galaxies; and analyses of redshift surveys both old and new. With the impending commencement of the Sloan Digital Sky Survey, presumably the definitive survey of nearby and moderate-redshift galaxies in our lifetime, the time is ripe for sober reflection of what has been recently accomplished and the directions that future research should take. The centerpiece of The Evolving Universe is the seminal review by A. Hamilton on linear-redshift distortions. Results are presented from the following surveys: The Norris Survey (Palomar), the MÃ1/4nster Redshift Project, the ESO Slice Project, Southern Sky Redshift Survey, CfA surveys and their extensions, Las Campanas Redshift Survey, CNOC, and CFRS. Theoretical analyses of luminosity functions, CMB-X Ray correlations, Cosmic String Models, Power Spectra, and quasar absorption line studies are also included. Audience: Scientists in the field as well as graduate students in astronomy will find The Evolving Universe to be a useful reference for current research as well as an explanation of the basic concepts of the field.
LC Classification Number
QB4-4.9
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