FUSE Measurements of Interstellar Fluorine
arXiv:astro-ph/0410362 · doi:10.1086/426778
Abstract
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 nu 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 A, absorption from H2 has to be modeled and then removed. Our analysis indicates that for H2 column densities less than about 3 x 10^20 cm^-2, the amount of F I can be determined from lambda 954. For these two sight lines, there is no clear indication for enhanced F abundances resulting from the nu process in a region shaped by past supernovae.
arXiv comment17 pages, 4 figures, accepted for publication in ApJ
References in corpus (9)
- The 'Forbidden' Abundance of Oxygen in the Sun
- Galactic Chemical Evolution: Hydrogen Through Zinc
- The Definitive Abundance of Interstellar Oxygen
- The Abundance of Interstellar Nitrogen
- Discovery of Interstellar Hydrogen Fluoride
- The Homogeneity of Interstellar Oxygen in the Galactic Disk
- Fluorine Abundances in the Large Magellanic Cloud and Omega Centauri: Evidence for Neutrino Nucleosynthesis?
- Cloud Structure and Physical Conditions in Star-forming Regions from Optical Observations. I. Data and Component Structure
- An Ultra-High-Resolution Survey of the Interstellar ^7Li-to-^6Li Isotope Ratio in the Solar Neighborhood
Cited by in corpus (29)
- The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
- Polycylcic Aromatic Hydrocarbons (PAH's) in dense cloud chemistry
- Ultraviolet Survey of CO and H_2 in Diffuse Molecular Clouds: The Reflection of Two Photochemistry Regimes in Abundance Relationships
- The chemistry of fluorine-bearing molecules in diffuse and dense interstellar gas clouds
- Fluorine and Sodium in C-rich low-metallicity stars
- The thermonuclear production of F19 by Wolf-Rayet stars revisited
- Fluorine in AGB Carbon Stars Revisited
- Fluorine abundances in planetary nebulae
- Effects of nuclear cross sections on F nucleosynthesis at low metallicities
- The Abundance of Interstellar Fluorine and Its Implications
- Fluorine in the solar neighborhood - is it all produced in AGB-stars?
- A new solar fluorine abundance and a fluorine determination in the two open clusters M 67 and NGC 6404
- Fluorine Abundances in the Orion Nebula Cluster
- Direct Determination of the HF/H2 Abundance Ratio in Interstellar Gas
- The impact of the 18F(a,p)21Ne reaction on asymptotic giant branch nucleosynthesis
- Discovery of Fluorine in Cool Extreme Helium Stars
- Fluorine abundances in dwarf stars of the solar neighbourhood
- Measurement of 1323 and 1487 keV resonances in 15N(α, γ)19F with the recoil separator ERNA
- Solar System Abundances and Condensation Temperatures of the Halogens Fluorine, Chlorine, Bromine, and Iodine
- Revisiting the Chlorine Abundance in Diffuse Interstellar Clouds from Measurements with the Copernicus Satellite
- Constraining -Process Production of Fluorine through Cosmic Ray Nucleosynthesis
- The fluorine abundance in a Galactic Bulge AGB star measured from CRIRES spectra
- The Abundance of Boron in Diffuse Interstellar Clouds
- Fluorine Abundances in the Galactic Nuclear Star Cluster
- First detection of AlF line emission towards M-type AGB stars
- The Nucleosynthesis and Reaction Rates of Fluorine 19 () in the Sun
- A Reexamination of Phosphorus and Chlorine Depletions in the Diffuse Interstellar Medium
- First detection of CF in the Large Magellanic Cloud
- The impact of the 18F(a,p)21Ne reaction on fluorine production in AGB stars