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Fluorine Abundances in Planetary Nebulae
Open accessAbstract
We have determined fluorine abundances from the [F II] λ4789 and [F IV] λ4060 nebular emission lines for a sample of planetary nebulae (PNe). Our results show that fluorine is generally overabundant in PNe, thus providing new evidence for the synthesis of fluorine in asymptotic giant branch (AGB) stars. [F/O] is found to be positively correlated with the C/O abundance ratio, in agreement with the predictions of theoretical models of fluorine production in thermally pulsing AGB stars. A large enhancement of fluorine is observed in the Wolf-Rayet PN NGC 40, suggesting that high mass-loss rates probably favor the survival of fluorine.
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Observationally, AGB stars and their progeny are the only confirmed site of F production.
“Observationally, AGB stars and their progeny (e.g., post-AGB stars, planetary nebulae) are the only confirmed site of F production (Jorissen et al. 1992; Werner et al. 2005; Zhang & Liu 2005; Pandey 2006; Schuler et al. 2007; Abia et al. 2010; Lucatello et al. 2011)”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Zhang & Liu 2005
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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
“…and their progeny (e.g., post-AGB stars, planetary nebulae) are the only confirmed site of F production (Jorissen et al. 1992; Werner et al. 2005; Zhang & Liu 2005; Pandey 2006; Schuler et al. 2007; Abia et al. 2010; Lucatello et al. 2011), with no clear indication for enhanced F abundances…”
Background
Metadata
- Authors
- Zhang, Y., & Liu, X.-W.
- Affiliations
- Space Telescope Science Institute (US)
- Peking University (CN)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2005-09-01
- Volume
- 631
- Issue
- 1
- Pages
- L61-L64
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1973167872
- Cited by
- 48
- References
- 0
- Citations by year
- 2025: 1 · 2024: 4 · 2023: 1 · 2022: 3 · 2021: 1 · 2020: 2 · 2019: 1 · 2018: 1 · 2017: 3 · 2015: 1 · 2014: 4 · 2013: 3 · 2012: 2
- FWCI
- 2.52
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
- The HKU Scholars Hub (University of Hong Kong) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Space Telescope Science Institute
- National Natural Science Foundation of China
- 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 abundance, planetary nebulae, asymptotic giant branch stars, C/O ratio, thermally pulsing AGB stars, mass loss, nebular abundances
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