Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 444, Issue 1, Pages 420-428Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stu1438
Keywords
atomic data; plasmas; radiation mechanisms: thermal; ISM: general; radio continuum: general
Categories
Funding
- Belgian Science Policy Office through the ESA PRODEX program
- NSF [1108928, 1109061, 1412155]
- NASA [10-ATP10-0053, 10-ADAP10-0073, NNX12AH73G, ATP13-0153]
- STScI [HST-AR-13245, GO-12560, HST-GO-12309, GO-13310.002-A]
- NASA [19755, NNX12AH73G] Funding Source: Federal RePORTER
- Direct For Mathematical & Physical Scien [1109061, 1412155] Funding Source: National Science Foundation
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [1108928] Funding Source: National Science Foundation
- Division Of Astronomical Sciences [1412155, 1109061] Funding Source: National Science Foundation
Ask authors/readers for more resources
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 (10)log is an element of(i) = -20 to +10 and (10)log w = -30 to +25. We then continued to produce a table of thermally averaged Gaunt factors covering the parameter space (10)log gamma(2) = -6 to +10 and (10)log u = -16 to +13. Finally, we produced a table of the frequency integrated Gaunt factor covering the parameter space (10)log gamma(2) = -6 to +10. All the data presented in this paper are available online.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available