RECENT UPDATE OF GAS-PHASE CHEMICAL REACTIONS AND MOLECULAR LINES OF TiO IN CLOUDY

We present our current update on the gas-phase chemical reactions and spectral lines of TiO in the spectral synthesis code Cloudy. For this purpose, we have added 229 Ti-related reactions in the chemical network. In addition, we consider 230 fine-structure energy levels, the corresponding 223 radiative transitions, and 444 collisional transitions with ortho and para H2, and predict 66 TiO lines. We perform spectroscopic simulations of TiO emission from the circumstellar region of the oxygen-rich red supergiant VY Canis Majoris to validate our update. Our model reproduces the observed TiO column density. This update is helpful in modeling dust-free astrophysical environments where Ti is in the gas phase and TiO can form.

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Publication Details

Journal
Revista Mexicana de Astronomía y Astrofísica
Published
2024-10-01
DOI
https://doi.org/10.22201/ia.01851101p.2024.60.02.15
Citations
1
Primary Topic
Gas Sensing Nanomaterials and Sensors
Type
article
Field-Weighted Citation Impact
0.21
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article

RECENT UPDATE OF GAS-PHASE CHEMICAL REACTIONS AND MOLECULAR LINES OF TiO IN CLOUDY

R. L. Porter, G. J. Ferland, P. C. Stancil, Gargi Shaw
1 citations
Revista Mexicana de Astronomía y Astrofísica
Gas Sensing Nanomaterials and Sensors
0.21
article

RECENT UPDATE OF GAS-PHASE CHEMICAL REACTIONS AND MOLECULAR LINES OF TiO IN CLOUDY

R. L. Porter, G. J. Ferland, P. C. Stancil, Gargi Shaw
article en
1 citations

Abstract

We present our current update on the gas-phase chemical reactions and spectral lines of TiO in the spectral synthesis code Cloudy. For this purpose, we have added 229 Ti-related reactions in the chemical network. In addition, we consider 230 fine-structure energy levels, the corresponding 223 radiative transitions, and 444 collisional transitions with ortho and para H2, and predict 66 TiO lines. We perform spectroscopic simulations of TiO emission from the circumstellar region of the oxygen-rich red supergiant VY Canis Majoris to validate our update. Our model reproduces the observed TiO column density. This update is helpful in modeling dust-free astrophysical environments where Ti is in the gas phase and TiO can form.

Revista Mexicana de Astronomía y AstrofísicaVol. 60(2)
Tata Institute of Fundamental Research (IN), University of Kentucky (US), University of Georgia (US), Stellar Science (United States) (US)
Affordable and clean energy
Openalex Percentile: Top 46%
Gas Sensing Nanomaterials and Sensors
0.21
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RECENT UPDATE OF GAS-PHASE CHEMICAL REACTIONS AND MOLECULAR LINES OF TiO IN CLOUDY — R. L. Porter, G. J. Ferland, et al. · Revista Mexicana de Astronomía y Astrofísica (2024) | TGRS Research Map | TGRS