Experimental study of the removal of excited state phosphorus atoms by HO and H: implications for the formation of PO in stellar winds
arXiv:2206.08193 · doi:10.1093/mnras/stac1684
Abstract
The reactions of the low-lying metastable states of atomic phosphorus, P(D) and P(P), with HO and H were studied by the pulsed laser photolysis at 248 nm of PCl , combined with laser induced fluorescence detection of P(D), P(P) and PO. Rate coefficients between 291 and 740 K were measured, along with a yield for the production of PO from P(D or P) + HO of (3515)%. H 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) to P(D), followed by reaction with HO, is a significant pathway for producing PO (in addition to the reaction between P(S) and OH). The model also demonstrates that the PN fractional abundance in a steady (non-pulsating) outflow is under-predicted by about 2 orders of magnitude. However, under shocked conditions where sufficient thermal dissociation of N occurs at temperatures above 4000 K, the resulting N atoms convert a substantial fraction of PO to PN.
24 pages, 7 figures, accepted for publication in MNRAS
References in corpus (7)
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- Phosphorus-bearing molecules in solar-type star forming regions: First PO detection
- The millimeter IRAM-30m line survey toward IK Tau
- Phosphorus-bearing molecules in the Galactic Center
- The first steps of Interstellar Phosphorus Chemistry
- Bottom-up dust nucleation theory in oxygen-rich evolved stars I. Aluminium oxide clusters
- Chemical complexity of phosphorous bearing species in various regions of the Interstellar medium
Cited by in corpus (3)
- ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA
- Bottom-up dust nucleation theory in oxygen-rich evolved stars II. Magnesium and calcium aluminate clusters
- New routes for PN destruction and formation in the ISM via neutral-neutral gas-phase reactions and an extended database for reactions involving phosphorus