Amanda Irene Karakas
research.monash.edu
0000-0002-3625-6951
Monash University
153 papers found
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Stellar Yields From Metal-Rich Asymptotic Giant Branch Models
The DIVERSE ORIGINS OF NEUTRON-CAPTURE ELEMENTS IN THE METAL-POOR STAR HD 94028: POSSIBLE DETECTION OF PRODUCTS OFi-PROCESS NUCLEOSYNTHESIS
On Potassium and Other Abundance Anomalies of Red Giants in Ngc 2419
On the nature of the most obscured C-rich AGB stars in the Magellanic Clouds
Current hot questions on the s process in AGB stars
The CHEMICAL ABUNDANCES OF STARS IN THE HALO (CASH) PROJECT. III. A NEW CLASSIFICATION SCHEME FOR CARBON-ENHANCED METAL-POOR STARS WITH S-Process ELEMENT ENHANCEMENT
Post-AGB stars in the Magellanic Clouds and neutron-capture processes in AGB stars
R Coronae Borealis Stars Are Viable Factories of Pre-Solar Grains
Division G Commission 35: Stellar Constitution
Evolution and nucleosynthesis of helium-rich asymptotic giant branch models
Monash chemical yields project (MonΧey) element production in low- and intermediate-mass stars
Evolution and Nucleosynthesis of Asymptotic Giant Branch Stellar Models of Low Metallicity
Helium enrichment and carbon-star production in metal-rich populations
Stellar origin of the 182Hf cosmochronometer and the presolar history of solar system matter
The Dawes Review 2: Nucleosynthesis and Stellar Yields of Low- and Intermediate-Mass Single Stars
The Aquarius comoving group is not a disrupted classical globular cluster★
恒星中子源13C(α, n)16O反应的研究
Slow neutron captures as the signature of asymptotic giant branch stars
The IMPACT OF UPDATED Zr NEUTRON-CAPTURE CROSS SECTIONS AND NEW ASYMPTOTIC GIANT BRANCH MODELS ON OUR UNDERSTANDING OF THESPROCESS AND THE ORIGIN OF STARDUST
On THE SOURCE OF THE DUST EXTINCTION IN TYPE Ia SUPERNOVAE AND THE DISCOVERY OF ANOMALOUSLY STRONG Na I ABSORPTION
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