Amanda Irene Karakas
research.monash.edu
0000-0002-3625-6951
Monash University
153 papers found
Refreshing results…
SALT reveals the barium central star of the planetary nebula Hen 2-39★
Hot bottom burning and s-process nucleosynthesis in massive AGB stars at the beginning of the thermally-pulsing phase
METAL-POOR STARS OBSERVED WITH THE MAGELLAN TELESCOPE. I. CONSTRAINTS ON PROGENITOR MASS AND METALLICITY OF AGB STARS UNDERGOINGs-PROCESS NUCLEOSYNTHESIS
3He: Does the problem persist?
Is the sulphur anomaly in planetary nebulae caused by the s-process?
LTE or non-LTE, that is the question
Nucleosynthesis in massive AGB stars with delayed superwinds: implications for the abundance anomalies in globular clusters .
Short-lived radioactivity in the early solar system: The Super-AGB star hypothesis
NEW DETERMINATION OF THE13C(α,n)16O REACTION RATE AND ITS INFLUENCE ON THEs-PROCESS NUCLEOSYNTHESIS IN AGB STARS
The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae
Publisher's Note: Reaction rates for thes-process neutron source22Ne +α[Phys. Rev. C85, 065809 (2012)]
Reaction rates for thes-process neutron source22Ne+α
The remarkable solar twin HIP 56948: a prime target in the quest for other Earths
Lithium Abundances in Carbon-Enhanced Metal-Poor Stars
Post-AGB stars in the SMC as tracers of stellar evolution: the extreme s-process enrichment of the 21 μm star J004441.04-732136.4
Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch Stars
The Curious Conundrum Regarding Sulfur Abundances in Planetary Nebulae
Rubidium, zirconium, and lithium production in intermediate-mass asymptotic giant branch stars
CNO and F abundances in the globular cluster M 22 (NGC 6656)
THEs-PROCESS IN ASYMPTOTIC GIANT BRANCH STARS OF LOW METALLICITY AND THE COMPOSITION OF CARBON-ENHANCED METAL-POOR STARS
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