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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3 Pith papers cite this work. Polarity classification is still indexing.
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Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
The paper proposes a comprehensive phase-space map of the Milky Way disk from existing and planned surveys plus a consortium to turn those data into a reconstruction of the galaxy's evolutionary history.
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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Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES
Six seismic solar analogs have masses 0.91-1.04 solar masses, radii 0.95-1.08 solar radii, and ages 1.8-9.1 Gyr, with one star matching the Sun closely enough to be called a solar twin.
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In Pursuit of Galactic Archaeology: Astro2020 Science White Paper
The paper proposes a comprehensive phase-space map of the Milky Way disk from existing and planned surveys plus a consortium to turn those data into a reconstruction of the galaxy's evolutionary history.