Identifiers
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name variant
H. J\"onsson
0.60 · backfill
Papers (15)
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The bimodal [Mg/Fe] versus [Fe/H] bulge sequence as revealed by APOGEE DR14
astro-ph.GA · 2019 · author #7
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4MOST: Project overview and information for the First Call for Proposals
astro-ph.IM · 2019 · author #158
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Abundances of disk and Bulge giants from high-resolution optical spectra III. Sc, V, Cr, Mn, Co, Ni
astro-ph.GA · 2019 · author #2
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A homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code. I. The Northern clusters
astro-ph.SR · 2018 · author #12
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Evidence against anomalous compositions for giants in the Galactic Nuclear Star Cluster
astro-ph.GA · 2018 · author #8
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A comprehensive comparison between APOGEE and LAMOST: Radial Velocities and Atmospheric Stellar Parameters
astro-ph.GA · 2018 · author #5
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Fluorine in the Solar Neighborhood: Chemical Evolution Models
astro-ph.GA · 2017 · author #3
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Detailed Abundances for the Old Population near the Galactic Center: I. Metallicity distribution of the Nuclear Star Cluster
astro-ph.GA · 2017 · author #7
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Baade's window with APOGEE: Metallicities, ages and chemical abundances
astro-ph.GA · 2017 · author #4
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Fluorine in the Solar neighborhood: No evidence for the neutrino process
astro-ph.SR · 2016 · author #1
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Abundances of disk and bulge giants from hi-res optical spectra: II. O, Mg, Ca, and Ti in the bulge sample
astro-ph.GA · 2016 · author #1
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Abundances of disk and bulge giants from hi-res optical spectra: I. O, Mg, Ca, and Ti in the Solar neighborhood and Kepler field samples
astro-ph.GA · 2016 · author #1
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Fluorine in the solar neighborhood - is it all produced in AGB-stars?
astro-ph.GA · 2014 · author #1
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The Chemical Evolution of Fluorine in the Bulge - High-resolution K-band spectra of giants in three fields
astro-ph.GA · 2014 · author #1
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Sulphur abundances in halo giants from the [S I] line at 1082 nm and the S I triplet around 1045 nm
astro-ph.GA · 2011 · author #1
Mentions
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1104.2148
#1 · backfill · confidence 0.70
H. J\"onsson