In this work, the chemi-ionization/recombination processes in tom- Rydberg atom collisions are considered as factors of influence on the ionization degree, atom excited-state populations and hydrogen molecule abundance in the dense moderately ionized regions in AGNs, as for example in clouds around the central black hole.
The obtained results demonstrate the fact that the considered chemi-ionization/recombination processes for principal quantum number $2 \le n \le 10$, and $5000\textrm{ K} \le T \le 12000\textrm{ K}$ must have certain influence on the optical properties of some parts of Narrow-Line Seyfert 1 Galaxies.
Volume 328 -
Revisiting narrow-line Seyfert 1 galaxies and their place in the Universe (NLS1-2018) -
Poster
Chemi-ionization processes in Narrow-Line Seyfert 1 Galaxies
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Pre-published on:
May 23, 2018
Published on:
December 21, 2018
Abstract
DOI: https://doi.org/10.22323/1.328.0049
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.