Evolution of Fluorine Abundances with the ν-Process

Abstract

We calculate the evolution of fluorine in the solar neighborhood with the ν-process of core-collapse supernovae, the results of which are in good agreement with the observations of field stars. The ν-process operating in supernovae causes the [F/O] ratio to plateau at [O/H] < -1.2, followed by a rapid increase toward [O/H] ~ -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.

4 pages, 1 figure, Accepted for publication in ApJL

References in corpus (8)

• Galactic chemical evolution: Carbon through Zinc
• Stellar Models and Yields of Asymptotic Giant Branch Stars
• Chemical abundances in giants stars of the tidally disrupted globular cluster NGC 6712 from high-resolution infrared spectroscopy
• Fluorine in carbon-enhanced metal-poor stars: a binary scenario
• Fluorine Abundances in the Milky Way Bulge
• The thermonuclear rate for the 19F(a,p)22Ne reaction at stellar temperatures
• nu-Process Nucleosynthesis in Population III Core-Collapse Supernovae
• Nucleosynthesis in High-Entropy Hot-Bubbles of SNe and Abundance Patterns of Extremely Metal-Poor Stars

Cited by in corpus (45)

• The Dawes Review 2: Nucleosynthesis and stellar yields of low and intermediate-mass single stars
• Chemical evolution with rotating massive star yields: I. The solar neighbourhood and the s-process elements
• The Most Metal-Poor Stars. II. Chemical Abundances of 190 Metal-Poor Stars Including 10 New Stars With [Fe/H] < -3.5
• Stellar yields from metal-rich asymptotic giant branch models
• NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01
• Systematic non-LTE study of the $-2.6\le$ [Fe/H] $\le 0.2$ F and G dwarfs in the solar neighbourhood. II. Abundance patterns from Li to Eu
• The Initial mass function of the first stars inferred from extremely metal-poor stars
• Iron-Group Abundances in the Metal-Poor Main Sequence Turnoff Star HD~84937
• Non standard s-process in massive rotating stars. Yields of $10-150$ $M_{\odot }$ models at $Z=10^{-3}$
• Principal Component Analysis on Chemical Abundances Spaces
• Planetary Nebulae: Sources of Enlightenment
• The Origin of Fluorine: Abundances in AGB Carbon Stars Revisited
• The $\nu$ process in the light of an improved understanding of supernova neutrino spectra
• Non-LTE analysis of K I in late-type stars
• Constraining cosmic scatter in the Galactic halo through a differential analysis of metal-poor stars
• Effects of nuclear cross sections on ${}^{19}$F nucleosynthesis at low metallicities
• CNO and F abundances in the globular cluster M22 (NGC 6656)
• The Chemical Evolution of Fluorine in the Bulge - High-resolution K-band spectra of giants in three fields
• Fluorine in the Solar neighborhood: No evidence for the neutrino process
• The $\nu$-process with fully time-dependent supernova neutrino emission spectra
• Fluorine in the solar neighborhood - is it all produced in AGB-stars?
• Fluorine in the Solar Neighborhood: Chemical Evolution Models
• Magnetic-buoyancy-induced mixing in AGB Stars: fluorine nucleosynthesis at different metallicities
• Origin of large meteoritic SiC stardust grains in metal-rich AGB stars
• Fingerprint of the first stars: multi-enriched extremely metal-poor stars in the TOPoS survey
• Fluorine in the solar neighborhood: modelling the Galactic thick and thin discs
• Fluorine Abundances of Galactic Low-Metallicity Giants
• Fluorine in the solar neighbourhood: the need for several cosmic sources
• Supernova Neutrino Process of Li and B Revisited
• The Abundance of Fluorine in Normal G and K Stars of the Galactic Thin Disk
• Neutrino self-interaction and MSW effects on the supernova neutrino-process
• Constraining $\nu$-Process Production of Fluorine through Cosmic Ray Nucleosynthesis
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• The ramp-up of interstellar medium enrichment at z>4
• Fluorine Abundances in the Galactic Disk
• Chemical Evolution of Fluorine in the Milky Way
• Fluorine Abundances in the Galactic Nuclear Star Cluster
• Search for Extremely Metal-Poor Stars with GEMINI-N/GRACES I. Chemical-Abundance Analysis
• The Nucleosynthesis and Reaction Rates of Fluorine 19 (${}^{19}F$) in the Sun
• Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine
• Exploring fluorine chemical evolution in the Galactic disk: the open cluster perspective
• The origin of elements: the need for UV spectra
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• Fluorine abundances in CEMP stars at the lowest metallicity: Hints on the nature of the first stars
• Fluorine Abundances in Local Stellar Populations