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On the origin of fluorine in the Milky Way
Open accessAbstract
The main astrophysical factories of fluorine (19F) are thought to be Type II supernovae, Wolf–Rayet stars, and the asymptotic giant branch (AGB) of intermediate‐mass stars. We present a model for the chemical evolution of fluorine in the Milky Way using a semi‐analytic multizone chemical evolution model. For the first time, we demonstrate quantitatively the impact of fluorine nucleosynthesis in Wolf–Rayet and AGB stars. The inclusion of these latter two fluorine production sites provides a possible solution to the long‐standing discrepancy between model predictions and the fluorine abundances observed in Milky Way giants. Finally, fluorine is discussed as a possible probe of the role of supernovae and intermediate‐mass stars in the chemical evolution history of the globular cluster ω Centauri.
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AGB stars are important for fluorine.
“Similarly, Renda et al. (2004) and Kobayashi et al. (2011a) showed the importance of AGB stars for fluorine.”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Renda et al. 2004
Core collapse supernovae and stellar winds from Wolf Rayet stars are predicted to release F-enriched material into the ISM, alongside AGB stars.
“Core collapse supernovae (Woosley & Weaver 1995) and stellar winds from Wolf Rayet stars (Meynet & Arnould 2000) are both predicted to release F-enriched material into the ISM, alongside AGB stars (Renda et al. 2004).”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Renda et al. 2004
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Cited by
Sorted by citations
The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars
Karakas, A. I., & Lattanzio, J. C. (2014) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2014.21 · Cited by 735
“Similarly, Renda et al. (2004) and Kobayashi et al. (2011a) showed the importance of AGB stars for fluorine.”
BackgroundSelf-citation
Metadata
- Authors
- Renda, A., Fenner, Y., Gibson, B. K., Karakas, A. I., Lattanzio, J. C., Campbell, S., Chieffi, A., Cunha, K., & Smith, V. V.
- Affiliations
- Swinburne University of Technology (AU)
- Monash University (AU)
- Astronomical Observatory of Rome (IT)
- The University of Texas at El Paso (US)
- Corresponding author
- Renda, Agostino
- ORCID
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2004-10
- Volume
- 354
- Issue
- 2
- Pages
- 575-580
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2083061365
- Cited by
- 92
- References
- 0
- Citations by year
- 2026: 1 · 2025: 5 · 2024: 4 · 2023: 3 · 2022: 5 · 2021: 3 · 2020: 5 · 2019: 4 · 2018: 4 · 2017: 4 · 2016: 1 · 2015: 2 · 2014: 6 · 2013: 3 · 2012: 2
- FWCI
- 4.33
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- Swinburne figshare (Swinburne University of Technology) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Keywords
- fluorine, 19F, chemical evolution, Milky Way, Wolf-Rayet stars, asymptotic giant branch, intermediate-mass stars, Type II supernovae, nucleosynthesis, giants, Omega Centauri, globular clusters
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