Search Results - "Gallagher, Andrew J."
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1
Candida guilliermondii/Kodamaea ohmeri Endocarditis
Published in Mycopathologia (1975) (01-12-2023)Get full text
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An Investigation of the Formation and Line Properties of MgH in 3D Hydrodynamical Model Stellar Atmospheres
Published in The Astrophysical journal (10-07-2017)“…Studies of the isotopic composition of magnesium in cool stars have so far relied upon the use of 1D model atmospheres. Since the isotopic ratios derived are…”
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A definition of and linguistic support for partial quiescence
Published in Concurrency and computation (10-06-2008)“…The global quiescence (GQ) of a distributed computation (or distributed termination detection) is an important problem. Some concurrent programming languages…”
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Generic operations and capabilities in the JR concurrent programming language
Published in Computer languages, systems & structures (01-10-2009)“…The JR concurrent programming language extends Java with additional concurrency mechanisms, which are built upon JR's operations and capabilities. JR…”
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Mono-enriched stars and Galactic chemical evolution -- Possible biases in observations and theory
Published 24-09-2020“…A&A 643, A49 (2020) A long sought after goal using chemical abundance patterns derived from metal-poor stars is to understand the Galactic chemical evolution…”
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Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars
Published 26-07-2019“…Manganese (Mn) is a key Fe-group elements, commonly employed in stellar population and nucleosynthesis studies to explore the role of SN Ia. We have developed…”
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Abundances in a sample of turnoff and subgiant stars in NGC 6121 (M4)
Published 11-08-2016“…{The aim of this work is to investigate the relations between the abundances of different elements in the globular cluster M4, selected for its uniform…”
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An investigation of the formation and line properties of MgH in 3D hydrodynamical model stellar atmospheres
Published 13-06-2017“…Studies of the isotopic composition of magnesium in cool stars have so far relied upon the use of one-dimensional (1D) model atmospheres. Since the isotopic…”
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Open Discussion
Published in The Annals of the American Academy of Political and Social Science (01-01-1915)Get full text
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