The DOI matches its Crossref record.
Far Ultraviolet Spectroscopic Explorer Measurements of Interstellar Fluorine
Open accessAbstract
The source of fluorine is not well understood, although core-collapse supernovae, Wolf-Rayet stars, and asymptotic giant branch stars have been suggested. A search for evidence of the ν-process during Type II supernovae is presented. Absorption from interstellar F I is seen in spectra of HD 208440 and HD 209339A acquired with the Far Ultraviolet Spectroscopic Explorer . In order to extract the column density for F I from the line at 954 Å, absorption from H 2 has to be modeled and then removed. Our analysis indicates that for H 2 column densities less than about 3 × 10 20 cm -2 , the amount of F I can be determined from λ954. For these two sight lines, there is no clear indication for enhanced F abundances resulting from the ν-process in a region shaped by past supernovae.
Overview
Integrity signals
Registry
Cites
Statistics
Verification
Claims the paper makes
Claims other papers make about this one
Each is checked against this paper’s own text: does it say what the citing paper says it does?
There is no clear indication for enhanced F abundances resulting from the ν-process in a region shaped by past SNe.
“with no clear indication for enhanced F abundances resulting from the ν -process in a region shaped by past SNe (Federman et al. 2005).”
From The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars (2014) · cites this paper as Federman et al. 2005
Citations
Cites
No references could be resolved yet.
Research works printed but not linked: 33
- 10.1086/322874 · DOI
- 10.1016/0016-7037(89)90286-X · DOI
- 10.1086/190850 · DOI
- 10.1086/423270 · DOI
- 10.1086/323440 · DOI
- 10.1086/377023 · DOI
- Danks A. C., 1984, A&A, 130, 62
- 10.1086/192052 · DOI
- 10.1086/159970 · DOI
- 10.1038/381764a0 · DOI
- 10.1023/A:1005161325181 · DOI
- Jorissen A., 1992, A&A, 261, 164
- 10.1086/346264 · DOI
- 10.1086/305235 · DOI
- 10.1046/j.1365-8711.1998.01361.x · DOI
- 10.1086/375492 · DOI
- Mowlavi N., 1998, A&A, 334, 153
- 10.1086/311023 · DOI
- 10.1086/305128 · DOI
- Meynet G., 2000, A&A, 355, 176
- 10.1086/377639 · DOI
- 10.1086/310942 · DOI
- 10.1086/381805 · DOI
- 10.1086/175912 · DOI
- 10.1086/306305 · DOI
- 10.1086/172098 · DOI
- 10.1086/172484 · DOI
- 10.1086/183585 · DOI
- 10.1086/192172 · DOI
- 10.1086/320354 · DOI
- 10.1086/168839 · DOI
- 10.1086/342240 · DOI
- 10.1086/309570 · DOI
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
“Kobayashi et al. (2011a) provide the most recent estimates of the chemical evolution of F using updated AGB yields as well as the latest ν-process yields from core-collapse SNe (see also Sánchez-Blázquez et al. 2012).”
BackgroundInfluential
Metadata
- Authors
- Federman, S. R., Sheffer, Y., Lambert, D. L., & Smith, V. V.
- Affiliations
- University of Toledo (US)
- McDonald Observatory (US)
- The University of Texas at El Paso (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2005-02
- Volume
- 619
- Issue
- 2
- Pages
- 884-890
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W1998695609
- Cited by
- 46
- References
- 0
- Citations by year
- 2025: 1 · 2024: 1 · 2023: 3 · 2022: 2 · 2019: 2 · 2017: 4 · 2014: 5 · 2013: 1 · 2012: 3
- FWCI
- 3.29
- 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)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- Johns Hopkins University
- Centre National d’Etudes Spatiales
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Keywords
- process, Type II supernovae, Wolf-Rayet stars, asymptotic giant branch stars, H2 column density, interstellar abundances
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
Are you an author, or do you see a problem with this page? Request a review
