Search Results - "KARAKAS, A. I"
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Updated stellar yields from asymptotic giant branch models
Published in Monthly notices of the Royal Astronomical Society (11-04-2010)“…An updated grid of stellar yields for low- to intermediate-mass thermally pulsing asymptotic giant branch (AGB) stars is presented. The models cover a range in…”
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On the formation of neutron stars via accretion-induced collapse in binaries
Published in Monthly notices of the Royal Astronomical Society (21-03-2019)Get full text
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The chemical compositions of solar twins in the open cluster M67
Published in Monthly notices of the Royal Astronomical Society (21-11-2016)“…Stars in open clusters are expected to share an identical abundance pattern. Establishing the level of chemical homogeneity in a given open cluster deserves…”
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The Large Magellanic Cloud as a laboratory for hot bottom burning in massive asymptotic giant branch stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2015)“…We use Spitzer observations of the rich population of asymptotic giant branch (AGB) stars in the Large Magellanic Cloud (LMC) to test models describing the…”
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Two distinct sequences of blue straggler stars in the globular cluster M 30
Published in Nature (London) (24-12-2009)“…Stars in globular clusters are generally believed to have all formed at the same time, early in the Galaxy's history. 'Blue stragglers' are stars massive…”
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EVOLUTION AND NUCLEOSYNTHESIS OF ASYMPTOTIC GIANT BRANCH STARS IN THREE MAGELLANIC CLOUD CLUSTERS
Published in The Astrophysical journal (10-02-2012)“…We present stellar evolutionary sequences for asymptotic giant branch (AGB) stars in the Magellanic Cloud clusters NGC 1978, NGC 1846, and NGC 419. The new…”
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On the nature of the most obscured C-rich AGB stars in the Magellanic Clouds
Published in Monthly notices of the Royal Astronomical Society (01-04-2016)“…The stars in the Magellanic Clouds with the largest degree of obscuration are used to probe the highly uncertain physics of stars in the asymptotic giant…”
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Double white dwarf mergers and elemental surface abundances in extreme helium and RCoronaeBorealis stars
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…ABSTRACT The surface abundances of extreme helium (EHe) and RCoronaeBorealis (RCB) stars are discussed in terms of a model for their origin in the merger of a…”
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The effect of including molecular opacities of variable composition on the evolution of intermediate-mass AGB stars
Published in Monthly notices of the Royal Astronomical Society (21-02-2014)“…Calculations from stellar evolutionary models of low- and intermediate-mass asymptotic giant branch (AGB) stars provide predictions of elemental abundances and…”
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The chemical evolution of globular clusters – I. Reactive elements and non-metals
Published in Monthly notices of the Royal Astronomical Society (11-05-2009)“…We propose a new chemical evolution model aimed at explaining the chemical properties of globular clusters (GCs) stars. Our model depends upon the existence of…”
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Rb-Rich Asymptotic Giant Branch Stars in the Magellanic Clouds
Published in The Astrophysical journal (01-11-2009)“…We present high-resolution (R approx 60,000) optical spectra of a carefully selected sample of heavily obscured and presumably massive O-rich asymptotic giant…”
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SALT reveals the barium central star of the planetary nebula Hen 2-39
Published in Monthly notices of the Royal Astronomical Society (21-12-2013)“…Classical barium stars are binary systems which consist of a late-type giant enriched in carbon and slow neutron capture (s-process) elements and an evolved…”
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Modelling self-pollution of globular clusters from asymptotic giant branch stars
Published in Monthly notices of the Royal Astronomical Society (01-09-2004)“…Abstract A self-consistent model of the chemical evolution of the globular cluster NGC 6752 is presented to test a popular theory that observed abundance…”
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The Chemical Evolution of Helium in Globular Clusters: Implications for the Self-Pollution Scenario
Published in The Astrophysical journal (01-12-2006)“…We investigate the suggestion that there are stellar populations in some globular clusters with enhanced helium (Y 6 0.28-0.40) compared to the primordial…”
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The 95Zr(n, γ)96Zr Cross Section from the Surrogate Ratio Method and Its Effect on s-process Nucleosynthesis
Published in The Astrophysical journal (20-10-2017)“…The 95Zr(n, γ)96Zr reaction cross section is crucial in the modeling of s-process nucleosynthesis in asymptotic giant branch stars because it controls the…”
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Iron and s-elements abundance variations in NGC 5286: comparison with ‘anomalous' globular clusters and Milky Way satellites
Published in Monthly notices of the Royal Astronomical Society (11-06-2015)“…We present a high-resolution spectroscopic analysis of 62 red giants in the Milky Way globular cluster (GC) NGC 5286. We have determined abundances of…”
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Heavy elements in barium stars
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT New elemental abundances for the neutron-capture elements Sr, Nb, Mo, Ru, La, Sm, and Eu are presented for a large sample of 180 barium (Ba) giant…”
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ON POTASSIUM AND OTHER ABUNDANCE ANOMALIES OF RED GIANTS IN NGC 2419
Published in The Astrophysical journal (10-02-2016)“…ABSTRACT Globular clusters are of paramount importance for testing theories of stellar evolution and early galaxy formation. Strong evidence for multiple…”
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Modelling of the post-asymptotic giant branch phase as a tool to understand asymptotic giant branch evolution and nucleosynthesis
Published in Monthly notices of the Royal Astronomical Society (01-02-2023)“…ABSTRACT We study a sample of single Galactic post-asymptotic giant branch (post-AGB) stars with known surface chemical composition. Gaia EDR3 and Gaia DR3…”
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The complex stellar system M 22: confirming abundance variations with high precision differential measurements
Published in Monthly notices of the Royal Astronomical Society (19-09-2022)“…ABSTRACT M 22 (NGC 6656) is a chemically complex globular cluster-like system reported to harbour heavy element abundance variations. However, the extent of…”
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