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Experimental study ...
Experimental study of the removal of excited state phosphorus atoms by H2O and H-2: implications for the formation of PO in stellar winds
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Douglas, K. M. (författare)
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- Gobrecht, David (författare)
- Gothenburg University,Göteborgs universitet,Institutionen för kemi och molekylärbiologi,Department of Chemistry and Molecular Biology
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Plane, J. M. C. (författare)
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(creator_code:org_t)
- 2022-06-21
- 2022
- Engelska.
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Ingår i: Monthly Notices of the Royal Astronomical Society. - : Oxford University Press (OUP). - 0035-8711 .- 1365-2966. ; 515:1, s. 99-109
- Relaterad länk:
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https://gup.ub.gu.se...
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https://doi.org/10.1...
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Abstract
Ämnesord
Stäng
- The reactions of the low-lying metastable states of atomic phosphorus, P(D-2) and P(P-2), with H2O and H-2 were studied by the pulsed laser photolysis at 248 nm of PCl3, combined with laser-induced fluorescence detection of P(D-2), P(P-2), and PO. Rate coefficients between 291 and 740 K were measured, along with a yield for the production of PO from P(D-2 or P-2) + H2O of (35 +/- 15) %. H-2 reacts with both excited P states relatively efficiently; physical (i.e. collisional) quenching, rather than chemical reaction to produced PH + H, is shown to be the more likely pathway. A comprehensive phosphorus chemistry network is then developed using a combination of electronic structure theory calculations and a Master Equation treatment of reactions taking place over complex potential energy surfaces. The resulting model shows that at the high temperatures within two stellar radii of a MIRA variable AGB star in oxygen-rich conditions, collisional excitation of ground-state P(S-4) to P(D-2), followed by reaction with H2O, is a significant pathway for producing PO (in addition to the reaction between P(S-4) and OH). The model also demonstrates that the PN fractional abundance in a steady (non-pulsating) outflow is underpredicted by about 2 orders of magnitude. However, under shocked conditions where sufficient thermal dissociation of N-2 occurs at temperatures above 4000 K, the resulting N atoms convert a substantial fraction of PO into PN.
Ämnesord
- NATURVETENSKAP -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
- NATURAL SCIENCES -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
Nyckelord
- astrochemistry
- molecular data
- methods: laboratory
- stars: wind
- outflows
- bearing molecules
- forming regions
- chemistry
- origin
- pn
- Astronomy & Astrophysics
Publikations- och innehållstyp
- ref (ämneskategori)
- art (ämneskategori)
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