3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
years
2026 3representative citing papers
Five O4 gravitational-wave events prefer dynamical cluster formation; typical recoil kicks eject remnants from globular clusters but allow possible retention in nuclear star clusters, disfavoring efficient hierarchical growth in globular clusters.
Direct N-body simulations independently confirm that preferential ejection of enriched RGB stars by an active black hole subsystem produces a transient overconcentration of pristine RGB stars in globular clusters that have lost substantial mass.
citing papers explorer
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3D NLTE Sodium abundances in late-type stars. Abundance corrections and synthetic spectra
3D NLTE sodium abundance corrections relative to 1D LTE are typically negative and larger for saturated lines in giants, reaching -0.7 dex, with a public grid released for use.
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Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers
Five O4 gravitational-wave events prefer dynamical cluster formation; typical recoil kicks eject remnants from globular clusters but allow possible retention in nuclear star clusters, disfavoring efficient hierarchical growth in globular clusters.
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Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem
Direct N-body simulations independently confirm that preferential ejection of enriched RGB stars by an active black hole subsystem produces a transient overconcentration of pristine RGB stars in globular clusters that have lost substantial mass.