The spectral energy distribution of galaxies : proceedings of the 284th Symposium of the International Astronomical Union held at the University of Central Lancashire, Preston, United Kingdom, September 5-9, 2011

書誌事項

The spectral energy distribution of galaxies : proceedings of the 284th Symposium of the International Astronomical Union held at the University of Central Lancashire, Preston, United Kingdom, September 5-9, 2011

edited by Richard J. Tuffs and Cristina C. Popescu

(IAU symposium and colloquium proceedings series, . IAU Symposium ; no. 284)

Cambridge University Press, 2012

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注記

At head of title: International Astronomical Union, Union Astronomique Internationale

Includes bibliographical references and author index

内容説明・目次

内容説明

Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma rays. This is motivating the development of new models for the interpretation of spectral energy distributions (SEDs) of galaxies in terms of the formation, evolution and emission of stellar and accretion-driven sources of photons, the interaction of the photons with the gaseous and dust components of the interstellar medium, and high-energy processes involving cosmic rays. IAU Symposium 284 details progress in the development of such models, their relation to fundamental theory, and their application to the interpretation of the panchromatic emission from the Milky Way and nearby galaxies, connecting the latter with models for the evolution of the SEDs of distant galaxies and the extragalactic background light. IAU S284 is a useful resource for all researchers working with the copious amounts of multiwavelength data for galaxies now becoming available.

目次

  • Preface
  • Introduction
  • Session 1. Population synthesis
  • Session 2. Understanding the emergent SEDs of local universe galaxies: 1. Spiral and dwarf galaxies
  • 2. Starburst galaxies and active galactic nuclei
  • 3. Early type galaxies
  • 4. Multiwavelength surveys
  • Session 3. Star-formation in galaxies
  • Session 4. The panchromatic view of the Milky Way
  • Session 5. Linking low- and high-energy properties of galaxies
  • Session 6. Understanding the cosmological evolution of emergent SEDs
  • Summary
  • Index.

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