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 language | English |
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Pages (from-to) | 420-428 |
Number of pages | 9 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 444 |
Issue number | 1 |
DOIs | |
State | Published - 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