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Comprehensive Coordination Chemistry II
  • Language: en
  • Pages: 11845

Comprehensive Coordination Chemistry II

  • Type: Book
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  • Published: 2003-12-03
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  • Publisher: Newnes

Comprehensive Coordination Chemistry II (CCC II) is the sequel to what has become a classic in the field, Comprehensive Coordination Chemistry, published in 1987. CCC II builds on the first and surveys new developments authoritatively in over 200 newly comissioned chapters, with an emphasis on current trends in biology, materials science and other areas of contemporary scientific interest.

Deep Fields
  • Language: en
  • Pages: 416

Deep Fields

This book is a synopsis of modern deep-field astronomy, based on the powerful telescopes and instruments developed in recent years. It is organized along topical themes, such as the extragalactic background radiation at different wavelengths, the evolution of galaxies, the history of star formation, the nature of absorbers, the reionization of the intergalactic medium, the validity of photometric redshifts, gravitational lensing, and clustering of galaxies. Stellar and substellar objects were not neglected, however, and one session was devoted to nearby bodies such as trans-Neptunian solar system objects, brown dwarfs, and stars with special characteristics.

Science with the VLT in the ELT Era
  • Language: en
  • Pages: 474

Science with the VLT in the ELT Era

The Workshop “Science with the VLT in the ELT Era” held in Garching from 8th to 12th October 2007 was organised by ESO, with support from its Scienti c and Technical Committee, to provide a forum for the astronomical community to debate the long term future of ESO’s Very Large Telescope (VLT) and its interferometric mode (VLTI). In particular it was considered useful for future planning to evaluate how its science use may evolve over the next decade due to competition and/or synergy with new facilities such as ALMA, JWST and, hopefully, at least one next generation 30–40 m extremely large telescope whose acronym appears in the title to symbolise this wider context. These discussions ...

The Impact of Large Scale Near-IR Sky Surveys
  • Language: en
  • Pages: 264

The Impact of Large Scale Near-IR Sky Surveys

After a year's successful operation, the European DENIS project is now a scientific reality and its close cousin 2MASS (USA) is about to come into operation. The observational and data reduction processes of both DENIS and 2MASS are fully described in this volume. Already the impact of DENIS is making itself felt in the astronomical community in areas of research as diverse as cosmology, the evolution of galaxies, the interstellar medium, the search for brown dwarfs, and stellar structure and evolution. The first routine results from DENIS and the preliminary results from the 2MASS prototype camera are discussed and compared with other surveys across the wavelength spectrum, both space- and ground-based, including the Digitized Sky Survey, ISO and ROSAT.

Euclid Preparation, [Bd.] XXI. Intermediate-redshift Contaminants in the Search for Z > 6 Galaxies Within the Euclid Deep Survey
  • Language: en

Euclid Preparation, [Bd.] XXI. Intermediate-redshift Contaminants in the Search for Z > 6 Galaxies Within the Euclid Deep Survey

  • Type: Book
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  • Published: 2022
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  • Publisher: Unknown

None

Scientific and Technical Aerospace Reports
  • Language: en
  • Pages: 248

Scientific and Technical Aerospace Reports

  • Type: Book
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  • Published: 1990
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  • Publisher: Unknown

None

Galaxy Evolution Across the Hubble Time (IAU S235)
  • Language: en
  • Pages: 480

Galaxy Evolution Across the Hubble Time (IAU S235)

This last decade has witnessed a revolution in our observations of galaxies; in particular deep imaging with HST and spectroscopy with 10m-class ground-based telescopes have uncovered many objects that are difficult to place along the Hubble sequence. High resolution spectroscopy of extremely faint objects has enabled the study of the kinematic evolution and, hence, the mass assembly of galaxies to unprecedented look-back times for direct comparison with cosmological structure formation scenarios. Thus, it is now possible to study all three aspects of galaxy evolution - their morphological-dynamical, chemical and spectral evolution out to redshift larger than six, exploring more than 95% of the age of the universe. These Proceedings of the IAU Symposium 235 report the considerable progress made in recent years on galaxy formation and evolution, and look forward to the expected breakthroughs in the domain of remote galaxies, with ALMA, the ELT and the next generation space telescopes.

Electron Paramagnetic Resonance
  • Language: en
  • Pages: 389

Electron Paramagnetic Resonance

Reflecting the growing volume of published work in this field, researchers will find this book an invaluable source of information on current methods and applications.

Advances in Catalysis
  • Language: en
  • Pages: 490

Advances in Catalysis

Catalysis is the acceleration of a chemical reaction by a catalyst, a substance that notably affects the rate of a chemical reaction without itself being consumed or altered. Since 1948, Advances in Catalysis has filled the gap between the papers that report on and the textbooks that teach in the diverse areas of catalysis research. The editors of and contributors to Advances in Catalysis are dedicated to recording progress in this area. Provides a comprehensive review of all aspects of catalytic research Contains in-depth, critical, state-of-the-art reports

A Panchromatic View of Galaxies
  • Language: en
  • Pages: 343

A Panchromatic View of Galaxies

Describing how to investigate all kinds of galaxies through a multifrequency analysis, this text is divided into three different sections. The first describes the data currently available at different frequencies, from X-rays to UV, optical, infrared and radio millimetric and centimetric, while explaining their physical meaning. In the second section, the author explains how these data can be used to determine physical parameters and quantities, such as mass and temperature. The final section is devoted to describing how the derived quantities can be used in a multifrequency analysis to study such physical processes as the star formation cycle and constrain models of galaxy evolution. As a result, observers will be able to interpret galaxies and their structure.