Accurate determination of the free-free gaunt factor - I. Non-relativistic gaunt factors

P. A.M. van Hoof, R. J.R. Williams, K. Volk, M. Chatzikos, G. J. Ferland, M. Lykins, R. L. Porter, Y. Wang

Research output: Contribution to journalArticlepeer-review

78 Scopus citations

Abstract

Modern spectral synthesis codes need the thermally averaged free-free Gaunt factor defined over a very wide range of parameter space in order to produce an accurate prediction for the spectrum emitted by an ionized plasma. Until now no set of data exists that would meet this need in a fully satisfactory way. We have therefore undertaken to produce a table of very accurate non-relativistic Gaunt factors over a much wider range of parameters than has ever been produced before. We first produced a table of non-averaged Gaunt factors, covering the parameter space 10log εi = -20 to +10 and 10log w = -30 to +25. We then continued to produce a table of thermally averaged Gaunt factors covering the parameter space 10log γ 2 = -6 to +10 and 10log u = -16 to +13. Finally, we produced a table of the frequency integrated Gaunt factor covering the parameter space 10log γ 2 = -6 to +10. All the data presented in this paper are available online.

Original languageEnglish
Pages (from-to)420-428
Number of pages9
JournalMonthly Notices of the Royal Astronomical Society
Volume444
Issue number1
DOIs
StatePublished - Jul 26 2014

Bibliographical note

Publisher Copyright:
© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society.

Keywords

  • Atomic data
  • ISM: general
  • Plasmas
  • Radiation mechanisms: thermal
  • Radio continuum: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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