65 citations · 79 across the 3 of their papers we have counts for
3 papers
astro-ph.SR2019★ 65 cited
Observational constraints on the origin of the elements II. 3D non-LTE formation of Ba ii lines in the solar atmosphere
A. J. Gallagher, M. Bergemann, R. Collet +5
Context. The pursuit of more realistic spectroscopic modelling and consistent abundances has led us to begin a new series of papers designed to improve current solar and stellar ab…
astro-ph.SR2019★ 14 cited
Be and O in the ultra metal-poor dwarf 2MASS J18082002-5104378: The Be-O correlation
M. Spite, P. Bonifacio, F. Spite +3
Measurable amounts of Be could have been synthesised primordially if the Universe were non-homogeneous or in the presence of late decaying relic particles. We investigate the Be ab…
astro-ph.SR2016
Enhanced methods for computing spectra from CO5BOLD models using Linfor3D. Molecular bands in metal-poor stars
A. J. Gallagher, M. Steffen, E. Caffau +3
Molecular features such as the G-band, CN-band and NH-band are important diagnostics for measuring a star's carbon and nitrogen abundances, especially in metal-poor stars where ato…