Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mnras.297.1073h&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 297, Issue 4, pp. 1073-1078.
Astronomy and Astrophysics
Astronomy
45
Atomic Data, Atomic Processes, Line: Formation
Scientific paper
A new calculation of photoionization cross-sections is described for the ground and excited states of atomic helium up to principal quantum number n=25 and angular momentum quantum number l=5. These cross-sections are used to calculate total recombination and cooling coefficients for atomic helium for electron temperatures given by log(T)=1(0.2)4.4. A comparison of the threshold photoionization cross-sections obtained here with extrapolations of the highly accurate bound-bound oscillator strength calculations by Drake shows that the new calculations are in error by no more than 1 per cent. The accuracy of the photoionization cross-sections used by previous workers to derive recombination coefficients is also discussed.
Hummer David G.
Storey Peter J.
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