Dielectronic Recombination of Fe 3 p q Ions: A Key Ingredient for Describing X-Ray Absorption in Active Galactic Nuclei-Reference-Cited by-同舟云学术

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Dielectronic Recombination of Fe 3 p q Ions: A Key Ingredient for Describing X-Ray Absorption in Active Galactic Nuclei

Published:2006-10-17 Issue:1 Volume:651 Page:L73-L76
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Badnell N. R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference21 articles.

1. Altun, Z., Yumak, A., Badnell, N. R., Loch, S. D. & Pindzola, M. S. 2006, A&A, submitted

2. Iron ionization and recombination rates and ionization equilibrium

3. Dielectronic recombination of Fe22+and Fe21+

4. Badnell, N. R. 2006a, J. Phys. B, in press (astro-ph/0607412)

5. Badnell, N. R. 2006b, ApJS, in press (astro-ph/0604144)

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2. Dielectronic recombination rate coefficients of carbon-like Kr³⁰⁺;Journal of Physics B: Atomic, Molecular and Optical Physics;2023-04-11

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4. Dielectronic recombination data for dynamic finite-density plasmas;Astronomy & Astrophysics;2022-12

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