HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure

Documenti analoghi

• HR-GO I: Comprehensive NLTE abundance analysis of the Cetus stream
  di: Sitnova, T. M., et al.
  Pubblicazione: (2024)
• Origin of $α$-Poor Very Metal-Poor Stars
  di: Jeena, S. K., et al.
  Pubblicazione: (2024)
• SDSSJ0018-0939: A Clear Signature of Sub-Chandrasekhar Mass Type 1a Supernova
  di: Jeena, S. K., et al.
  Pubblicazione: (2024)
• The Pristine Inner Galaxy Survey (PIGS) IX. The largest detailed chemical analysis of very metal-poor stars in the Sagittarius dwarf galaxy
  di: Sestito, Federico, et al.
  Pubblicazione: (2024)
• Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties
  di: Zhang, Ruizhi, et al.
  Pubblicazione: (2024)