Afficher la notice abrégée

dc.contributor.authorCAMPANHA, Danilo R.
dc.contributor.authorMENDOZA, Edgar
dc.contributor.authorSILVA, Mateus X.
dc.contributor.authorVELLOSO, Paulo F. G.
dc.contributor.authorCARVAJAL, Miguel
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorWAKELAM, Valentine
dc.contributor.authorGALVÃO, Breno R. L.
dc.date.issued2022
dc.identifier.issn0035-8711
dc.description.abstractEnThe Si + SO<SUB>2</SUB> reaction is investigated to verify its impact on the abundances of molecules with astrochemical interest, such as SiS, SiO, SO, and others. According to our results Si(<SUP>3</SUP>P) and SO<SUB>2</SUB> react barrierlessly yielding only the monoxides SO and SiO as products. No favourable pathway has been found leading to other products, and this reaction should not contribute to SiS abundance. Furthermore, it is predicted that SiS is stable in collisions with O<SUB>2</SUB>, and that S(<SUP>3</SUP>P) + SiO<SUB>2</SUB> and O(<SUP>3</SUP>P)+OSiS will also produce SO + SiO. Using these results and gathering further experimental and computational data from the literature, we provide an extended network of neutral-neutral reactions involving Si- and S-bearing molecules. The effects of these reactions were examined in a protostellar shock model, using the NAUTILUS gas-grain code. This consisted in simulating the physicochemical conditions of a shocked gas evolving from (i) primeval cold core, (ii) the shock region itself, (iii) and finally the gas bulk conditions after the passage of the shock. Emphasizing on the cloud ages and including systematically these chemical reactions, we found that [SiS/H<SUB>2</SUB>] can be of the order of ~10<SUP>-8</SUP> in shocks that evolves from clouds of t = 1 × 10<SUP>6</SUP> yr, whose values are mostly affected by the SiS + O $\longrightarrow$SiO + S reaction. Perspectives on further models along with observations are discussed in the context of sources harbouring molecular outflows.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enastrochemistry
dc.subject.enmolecular data
dc.subject.enISM: abundances
dc.subject.enISM: evolution
dc.subject.enISM: molecules
dc.subject.enAstrophysics - Astrophysics of Galaxies
dc.title.enThe Si + SO<SUB>2</SUB> collision and an extended network of neutral-neutral reactions between silicon and sulphur bearing species
dc.typeArticle de revue
dc.identifier.doi10.1093/mnras/stac1647
dc.subject.halPlanète et Univers [physics]
dc.identifier.arxiv2206.04982
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.page369-377
bordeaux.volume515
bordeaux.peerReviewedoui
hal.identifierinsu-03868236
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//insu-03868236v1
bordeaux.COinSctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.jtitle=Monthly%20Notices%20of%20the%20Royal%20Astronomical%20Society&amp;rft.date=2022&amp;rft.volume=515&amp;rft.spage=369-377&amp;rft.epage=369-377&amp;rft.eissn=0035-8711&amp;rft.issn=0035-8711&amp;rft.au=CAMPANHA,%20Danilo%20R.&amp;MENDOZA,%20Edgar&amp;SILVA,%20Mateus%20X.&amp;VELLOSO,%20Paulo%20F.%20G.&amp;CARVAJAL,%20Miguel&amp;rft.genre=article


Fichier(s) constituant ce document

FichiersTailleFormatVue

Il n'y a pas de fichiers associés à ce document.

Ce document figure dans la(les) collection(s) suivante(s)

Afficher la notice abrégée