2016A&A...587A..84M


Query : 2016A&A...587A..84M

2016A&A...587A..84M - Astronomy and Astrophysics, volume 587A, 84-84 (2016/3-1)

Parameterization of the level-resolved radiative recombination rate coefficients for the SPEX code.

MAO J. and KAASTRA J.

Abstract (from CDS):

The level-resolved radiative recombination (RR) rate coefficients for H-like to Na-like ions from H (Z=1) up to and including Zn (Z=30) are studied here. For H-like ions, the quantum-mechanical exact photoionization cross sections for nonrelativistic hydrogenic systems are usedto calculate the RR rate coefficients under the principle of detailed balance, while for He-like to Na-like ions, the archival data on ADAS are adopted. Parameterizations are made for the direct capture rates in a wide temperature range. The fitting accuracies are better than 5% for about 99% of the ∼3x104 levels considered here. The ∼1% exceptions include levels from low-charged many-electron ions, and/or high-shell (n>4) levels are less important in terms of interpreting X-ray emitting astrophysical plasmas. The RR data will be incorporated into the high-resolution spectral analysis package SPEX.

Abstract Copyright:

Journal keyword(s): atomic data - atomic processes

VizieR on-line data: <Available at CDS (J/A+A/587/A84): rr_spex3.dat>

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2022.12.07-03:51:17

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