Issue |
A&A
Volume 665, September 2022
|
|
---|---|---|
Article Number | A94 | |
Number of page(s) | 25 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/202142305 | |
Published online | 19 September 2022 |
Inverted level populations of hydrogen atoms in ionized gas
1
Shanghai Astronomical Observatory, Chinese Academy of Sciences,
80 Nandan Road,
Shanghai,
200030, PR China
e-mail: [email protected]; [email protected]
2
Research Center for Intelligent Computing Platforms, Zhejiang Laboratory,
Hangzhou
311100, PR China
3
School of Physical Science and Technology, Guangxi University,
Nanning
530004, PR China
4
Department of Astronomy, University of Science and technology of China,
Hefei
230026, PR China
5
Physics Department, Guangzhou University,
Guangzhou
510006, PR China
Received:
24
September
2021
Accepted:
22
May
2022
Context. Level population inversion of hydrogen atoms in ionized gas may lead to stimulated emission of hydrogen recombination lines, and the level populations can in turn be affected by powerful stimulated emissions.
Aims. In this work the interaction of the radiation fields and the level population inversion of hydrogen atoms is studied. The effect of the stimulated emissions on the line profiles is also investigated.
Methods. Our previous nl-model for calculating level populations of hydrogen atoms and hydrogen recombination lines is improved. The effects of line and continuum radiation fields on the level populations are considered in the improved model. By using this method the properties of simulated hydrogen recombination lines and level populations are used in analyses.
Results. The simulations show that hydrogen radio recombination lines are often emitted from the energy level with an inverted population. The widths of Hnα lines can be significantly narrowed by strong stimulated emissions to be even less than 10 km s−1. The amplification of hydrogen recombination lines is more affected by the line optical depth than by the total optical depth. The influence of stimulated emission on the estimates of electron temperature and density of ionized gas is evaluated. We find that comparing multiple line-to-continuum ratios is a reliable method for estimating the electron temperature, while the effectiveness of the estimation of electron density is determined by the relative significance of stimulated emission.
Key words: line: profiles / methods: numerical / stars: massive / HII regions / radio lines: ISM
© F.-Y. Zhu et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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