Determination of effective temperatures for an extended sample of dwarfs and subdwarfs (F0-K5)
Astron. Astrophys. Suppl. Ser., 117 2 (1996) 227-254
Published online: 1996-06-15
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A Search for Nitrogen‐enhanced Metal‐poor Stars
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Medium-resolution Isaac Newton Telescope library of empirical spectra ? II. The stellar atmospheric parameters
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The Distances to Open Clusters from Main‐Sequence Fitting. IV. Galactic Cepheids, the LMC, and the Local Distance Scale
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The Distances to Open Clusters from Main‐Sequence Fitting. III. Improved Accuracy with Empirically Calibrated Isochrones
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Sulphur abundances from the S i near-infrared triplet at 1045 nm
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Non-LTE Balmer line formation in late-type spectra: effects of atomic processes involving hydrogen atoms
P. S. BarklemAstronomy & Astrophysics 466 (1) 327 (2007)
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The helium abundance and ΔY/ΔZ in lower main-sequence stars
Luca Casagrande, Chris Flynn, Laura Portinari, Leo Girardi and Raul JimenezMonthly Notices of the Royal Astronomical Society 382 (4) 1516 (2007)
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Element abundances of unevolved stars in the open cluster M 67
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Accurate fundamental parameters for lower main-sequence stars
Luca Casagrande, Laura Portinari and Chris FlynnMonthly Notices of the Royal Astronomical Society 373 (1) 13 (2006)
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Revisiting two local constraints of the Galactic chemical evolution
M. HaywoodMonthly Notices of the Royal Astronomical Society 371 (4) 1760 (2006)
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Oxygen from the λ7774 High‐Excitation Triplet in Open Cluster Dwarfs: Hyades
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Basic physical parameters of a selected sample of evolved stars
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Effective temperature scale and bolometric corrections from 2MASS photometry
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