2025MNRAS.538.2693M


Query : 2025MNRAS.538.2693M

2025MNRAS.538.2693M - Mon. Not. R. Astron. Soc., 538, 2693-2703 (2025/April-3)

R-matrix calculations of photoionization cross-sections of sulfur-containing compounds.

MAHLA S. and ANTONY B.

Abstract (from CDS):

In this work, the R-matrix method was employed to calculate the total and partial-channel photoionization cross-sections for the initial three bands of hydrogen sulfide ($\mathrm{H_2S}$), four bands of carbon disulfide ($\mathrm{CS_2}$), and three bands of carbonyl sulfide ($\mathrm{OCS}$) molecules. These calculations were performed over the entire range of photon energy, starting from the ionization thresholds of the respective states and extending significantly beyond the final level thresholds of the target ions. The present computations are performed within the fixed-nuclei approximation, which does not consider vibration or rotation. However, it incorporates electron correlation effects and resonant photoionization contributions that have not been considered in any previously published literature. Intense absorption is observed in the total photoionization cross-section at energies below 20 eV, with a significant portion of it being caused by the excitation of molecules that subsequently decay by strong autoionization. These are assigned to Rydberg levels strengthened by the remarkably extensive partial photoionization of the $\left(2 b_1^{-1}\right) \mathrm{X}^2 \mathrm{B_1}$ channel in $\mathrm{H_2S}$, $\left(2 \pi _g^{-1}\right) \mathrm{X}^2 \mathrm{\Pi _g}$ channel in $\mathrm{CS_2}$, and $\left(3 \pi ^{-1}\right) \mathrm{X}^2 \mathrm{\Pi }$ channel in $\mathrm{OCS}$, within the 10-16 eV excitation range. The current R-matrix results are mostly in line with previous experimental measurements and theoretical calculations. There are some differences, though, which can be explained by the large number of Rydberg resonances just above the photoionization threshold. The computed data are crucial for modelling parameters observed in photoionized plasmas.

Abstract Copyright: © 2025 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): molecular data - molecular processes - radiation mechanisms: general - scattering - methods: numerical

Simbad objects: 12

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Number of rows : 12
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NGC 253 SyG 00 47 33.134 -25 17 19.68   8.03   6.94 8.1 ~ 3588 2
2 W 3 MoC 02 27 04.10 +61 52 27.1           ~ 1064 3
3 TMC-1 MoC 04 41 45.9 +25 41 27           ~ 1872 0
4 NAME OMC-1 MoC 05 35 14 -05 22.4           ~ 1249 2
5 NAME Orion Core ? 05 35 14.5 -05 22 30           ~ 212 0
6 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
7 M 82 AGN 09 55 52.430 +69 40 46.93 9.61 9.30 8.41     ~ 6156 6
8 LDN 183 MoC 15 54 12.2 -02 49 42           ~ 799 1
9 NAME Sgr B2 MoC 17 47 20.4 -28 23 07           ~ 2443 1
10 W 33a Y*O 18 14 39.56547 -17 52 02.2260           ~ 746 0
11 W 51 SNR 19 23 50 +14 06.0           ~ 1352 1
12 NGC 7538 OpC 23 13 37 +61 30.0           ~ 920 1

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