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dc.contributor.authorKobayashi, Chiaki
dc.contributor.authorIzutani, Natsuko
dc.contributor.authorKarakas, Amanda I.
dc.contributor.authorYoshida, Takashi
dc.contributor.authorYong, David
dc.contributor.authorUmeda, Hideyuki
dc.date.accessioned2011-12-20T13:01:02Z
dc.date.available2011-12-20T13:01:02Z
dc.date.issued2011-10-01
dc.identifier.citationKobayashi , C , Izutani , N , Karakas , A I , Yoshida , T , Yong , D & Umeda , H 2011 , ' Evolution of fluorine in the galaxy with the v-process ' , Astrophysical Journal Letters , vol. 739 , no. 2 , L57 . https://doi.org/10.1088/2041-8205/739/2/L57
dc.identifier.issn2041-8213
dc.identifier.otherPURE: 492564
dc.identifier.otherPURE UUID: 8a00d9c9-899a-4680-ae43-6cefff3d0211
dc.identifier.otherWOS: 000294997600023
dc.identifier.otherScopus: 80053479386
dc.identifier.otherORCID: /0000-0002-4343-0487/work/62750435
dc.identifier.urihttp://hdl.handle.net/2299/7409
dc.description.abstractWe calculate the evolution of fluorine in the solar neighborhood with the v-process of core-collapse supernovae, the results of which are in good agreement with the observations of field stars. The v-process operating in supernovae causes the [F/O] ratio to plateau at [O/H] less than or similar to-1.2,followed by a rapid increase toward [O/H] similar to-0.5 from the contribution of asymptotic giant branch stars. The plateau value of [F/O] depends on the neutrino luminosity released by core-collapse supernovae and may be constrained by using future observations of field stars at low metallicities. For globular clusters, the handful of [F/O] measurements suggest that the relative contribution from low-mass supernovae is smaller in these systems than in the field.en
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Letters
dc.subjectGalaxy: abundances
dc.subjectGalaxy: evolution
dc.subjectstars: abundances
dc.subjectstars: AGB and post-AGB
dc.subjectsupernovae: general
dc.subjectGALACTIC CHEMICAL EVOLUTION
dc.subjectGIANT BRANCH STARS
dc.subjectPOPULATION-III SUPERNOVAE
dc.subjectCORE-COLLAPSE SUPERNOVAE
dc.subjectR-PROCESS ELEMENTS
dc.subjectMETAL-POOR STARS
dc.subjectWOLF-RAYET STARS
dc.subjectMASSIVE STARS
dc.subjectMILKY-WAY
dc.subjectNEUTRINO NUCLEOSYNTHESIS
dc.titleEvolution of fluorine in the galaxy with the v-processen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
dc.identifier.urlhttp://www.scopus.com/inward/record.url?scp=80053479386&partnerID=8YFLogxK
rioxxterms.versionSMUR
rioxxterms.versionofrecordhttps://doi.org/10.1088/2041-8205/739/2/L57
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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