Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. III. Si‐Sequence Ions: Si i , S iii , Ar v , Ca vii , and Fe xiii-Reference-Cited by-同舟云学术

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Electron‐Ion Recombination Rate Coefficients and Photoionization Cross Sections for Astrophysically Abundant Elements. III. Si‐Sequence Ions: Si i , S iii , Ar v , Ca vii , and Fe xiii

Published:2000-02 Issue:2 Volume:126 Page:537-550
ISSN:0067-0049
Container-title:The Astrophysical Journal Supplement Series
language:en
Short-container-title:ASTROPHYS J SUPPL S

Author:

Nahar Sultana N.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

1. Dielectronic recombination. I. General theory

2. Atomic data for opacity calculations. II. Computational methods

3. A General Formula for the Estimation of Dielectronic Recombination Co-Efficients in Low-Density Plasmas.

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