Pith. sign in

REVIEW

Phosphorous chemistry in the shocked region L1157 B1

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1210.7900 v1 pith:IT4GLHDJ submitted 2012-10-30 astro-ph.SR astro-ph.GA

classification astro-ph.SRastro-ph.GA
keywords abundancepre-shockspeciesatomsc-shockchemistryelementalfind
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

We study the evolution of phosphorous-bearing species in one-dimensional C-shock models. We find that the abundances of P-bearing species depend sensitively on the elemental abundance of P in the gas phase and on the abundance of N atoms in the pre-shock gas. The observed abundance of PN and the non-detection of PO towards L1157 B1 are reproduced in C-shock models with shock velocity v=20km s-1 and pre-shock density n(H2) =10^4 - 10^5, if the elemental abundance of P in the gas phase is 10^-9 and the N-atom abundance is n(N)/nH - 10^-5 in the pre-shock gas. We also find that P-chemistry is sensitive to O- and N-chemistry, because N atoms are destroyed mainly by OH and NO. We identify the reactions of O-bearing and N-bearing species that significantly affect P chemistry.

Discussion (0). Sign in to comment.

Pith tools