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  3. The Analysis of Emission Lines
  • Cited by 5
      • Edited by Robert Williams, Space Telescope Science Institute, Baltimore, Mario Livio, Space Telescope Science Institute, Baltimore
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    • Publisher:
      Cambridge University Press
      Publication date:
      November 2009
      October 1995
      ISBN:
      9780511600180
      9780521480819
      9780521675604
      DOI:
      https://doi.org/10.1017/CBO9780511600180
      Dimensions:
      (247 x 174 mm)
      Weight & Pages:
      0.646kg, 236 Pages
      Dimensions:
      (247 x 174 mm)
      Weight & Pages:
      0.385kg, 236 Pages
      • Subjects:
      Observational Astronomy, Techniques and Instrumentation, Physics and Astronomy, Astronomy: General Interest
      Series:
      Space Telescope Science Institute Symposium Series (8)
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    • Selected: Digital
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    Subjects:
    Observational Astronomy, Techniques and Instrumentation, Physics and Astronomy, Astronomy: General Interest
    Series:
    Space Telescope Science Institute Symposium Series (8)
    Information

    Book description

    What can emission lines tell us about an astrophysical object? A workshop at the Space Telescope Science Institute was dedicated to address just this question – for a host of objects (including planetary nebulae and active galactic nuclei) across a broad range of wavelengths (from the infrared through to gamma-rays). Thirteen review articles from internationally renowned experts are presented in this volume. They provide an edited and coherent overview of the latest technical data, techniques in and applications of the study of emission lines from a variety of objects. Chapters include the theory of radiative transfer, photoionising shocks, and emission lines from stellar winds, as well as useful summaries of abundance determinations, atomic data, and diagnostics for IR, UV, gamma-ray and molecular lines. Together these review articles provide an overview of the analysis of emission lines. They summarise current knowledge, highlight outstanding problems and provide focus for fruitful future research. In this way they provide an excellent introduction for graduate students and reference for professionals.

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    Contents

    Contents
    • The Lexington Benchmarks for Numerical Simulations of Nebulae
      pp 83-96
      • By G. Ferland, Physics and Astronomy, University of Kentucky, Lexington, KY 40506, gary@cloud9. pa.uky. edu, L. Binette, ESO, D-85748, Garching bei Muenchen, Germany, lbinette@eso.org, M. Contini, School of Physics and Astronomy, Tel Aviv University, 69978 Tel Aviv, Israel, netzer@wise.tau. ac. il, contini@ccsg. tau. ac.il, J. Harrington, 4Astronomy, U of Maryland, College Park, MD 20742, jph@astro.umd.edu, T. Kallman, Code 665, NASA Goddard SFC, Greenbelt, MD 20771, tim@xstar.gsfc.nasa.gov, H. Netzer, School of Physics and Astronomy, Tel Aviv University, 69978 Tel Aviv, Israel, netzer@wise.tau. ac. il, contini@ccsg. tau. ac.il, D. Péquignot, Observatoire de Paris, Meudon F-92195, Meudon Principal Cedex, France, pequignot@obspm.fr, J. Raymond, CfA, 60 Garden St., Cambridge, MA 02138, raymond@cfassp8.harvard.edu, R. Rubin, NASA/Ames Research Center, MS 245-6, Moffett Field, CA 94035-1000, rubin@cygnus. arc.nasa.gov, G. Shields, Astronomy, University of Texas, Austin, TX 78712, shields@astro.as.utexas.edu, R. Sutherland, JILA, University of Colorado, Boulder, CO 80309-0440, ralph@zwicky.colorado.edu, S. Viegas, AGUSP, Av. Miguel Stefano 4200, 04301 Sao Paulo, S.P., Brazil, viegas@iag.usp.ansp.br

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