Pismis 18 is an intermediate-age (~700 Myr) inner-disc open cluster at ~7 kpc Galactocentric distance with [Fe/H] = +0.23, slightly super-solar [α/Fe] and s-process elements, and updated parameters from high-confidence members.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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astro-ph.SR 2years
2019 2representative citing papers
Uniform atmospheric parameters (Teff, log g, [Fe/H]) derived for 616 XSL stars via ULySS fitting to MILES, with reported precisions of 0.9-2.6% in Teff depending on stellar type.
citing papers explorer
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The Gaia-ESO Survey: The inner disc, intermediate-age open cluster Pismis 18
Pismis 18 is an intermediate-age (~700 Myr) inner-disc open cluster at ~7 kpc Galactocentric distance with [Fe/H] = +0.23, slightly super-solar [α/Fe] and s-process elements, and updated parameters from high-confidence members.
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Stellar atmospheric parameters for 754 spectra from the X-shooter Spectral Library
Uniform atmospheric parameters (Teff, log g, [Fe/H]) derived for 616 XSL stars via ULySS fitting to MILES, with reported precisions of 0.9-2.6% in Teff depending on stellar type.