about
Two distinct sequences of blue straggler stars in the globular cluster M 30.Early solar system. Stellar origin of the ¹⁸²Hf cosmochronometer and the presolar history of solar system matter.On the origin of fluorine in the Milky WayThe R-Process Alliance: Discovery of the First Metal-poor Star with a Combined r- and s-process Element SignatureThe Chemical Abundances of Stars in the Halo (CASH) Project. III. A new classification scheme for carbon-enhanced metal-poor stars with s-process element enhancementTungsten isotopic compositions in stardust SiC grains from the murchison meteorite: constraints on the s-process in the Hf-Ta-W-Re-Os regionOn the source of the dust extinction in type Ia supernovae and the discovery of anomalously strong Na I absorptionUncertainties in AGB evolution and nucleosynthesisStellar yields from metal-rich asymptotic giant branch modelsThe diverse origins of neutron-capture elements in the metal-poor star HD 94028: possible detection of products of i-process nucleosynthesisHigh-precision analysis of the solar twin HIP 100963Evolution and nucleosynthesis of helium-rich asymptotic giant branch modelsHIP 10725: The first solar twin/analogue field blue stragglerMonash Chemical Yields Project (Monχey) Element production in low- and intermediate-mass starsR Coronae Borealis stars are viable factories of pre-solar grainsStellar yields – theory and observations18 Sco: A SOLAR TWIN RICH IN REFRACTORY AND NEUTRON-CAPTURE ELEMENTS. IMPLICATIONS FOR CHEMICAL TAGGINGChemical abundances in bright giants of the globular cluster M62 (NGC 6266)★Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicityHelium enrichment and carbon-star production in metal-rich populationsIron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089)★Nucleosynthesis in helium-enriched asymptotic giant branch models: implications for heavy element enrichment in {omega} CentauriThe Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single StarsThe impact of updated zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the s process and the origin of stardustTHEs-PROCESS ENRICHMENT OF THE GLOBULAR CLUSTERS M4 AND M22Is the sulphur anomaly in planetary nebulae caused by the s-process?Metal-poor stars observed with the Magellan telescope. I. Constraints on progenitor mass and metallicity of AGB stars undergoing s-process nucleosynthesisCarbon-enhanced metal-poor stars and the s/r processHeavy element nucleosynthesis in the brightest galactic asymptotic giant branch starsLithium abundances in carbon-enhanced metal-poor starsShort-lived radioactivity in the early solar system: The Super-AGB star hypothesisThe curious conundrum regarding sulfur abundances in planetary nebulaeThe s-process at low metallicityTHEs-PROCESS IN ASYMPTOTIC GIANT BRANCH STARS OF LOW METALLICITY AND THE COMPOSITION OF CARBON-ENHANCED METAL-POOR STARSThe curious conundrum regarding sulfur and oxygen abundances in planetary nebulaeThe evolution of isotope ratios in the Milky Way GalaxyHeavy Element Abundances in Planetary Nebulae: A Theorist's PerspectiveIs extra mixing really needed in asymptotic giant branch stars?The slow-neutron capture process in low-metallicity asymptotic giant branch starsThe ubiquity of the rapid neutron-capture process
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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Amanda I. Karakas
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P21
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0000-0002-3625-6951