JINA - Segue Virtual Journal, 10 June 2022
Volume 17, Issue 23 (11 Articles)
- # 1 - An old, metal-rich accreted stellar component in the Milky Way stellar disk. (arXiv:2206.03875v1 [astro-ph.GA])
- # 2 - On the inconsistency of [C/Fe] abundances and the fractions of carbon-enhanced metal-poor stars among various stellar surveys. (arXiv:2206.04081v1 [astro-ph.GA])
- # 3 - Origin of Highly $r$-Process-Enhanced Stars in a Cosmological Zoom-in Simulation of a Milky Way-like Galaxy. (arXiv:2206.04060v1 [astro-ph.GA])
- # 4 - The chemical enrichment of the Milky Way disk evaluated using conditional abundances. (arXiv:2206.02772v1 [astro-ph.GA])
- # 5 - The disturbed outer Milky Way disc. (arXiv:2206.04059v1 [astro-ph.GA])
- # 6 - The missing radial velocities of Gaia: blind predictions for DR3. (arXiv:2206.04102v1 [astro-ph.GA])
- # 7 - The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers. (arXiv:2206.04521v1 [astro-ph.GA])
- # 8 - The stellar halo in Local Group Hestia simulations II. The accreted component. (arXiv:2206.04522v1 [astro-ph.GA])
- # 9 - From dawn till disc: Milky Way’s turbulent youth revealed by the APOGEE+Gaia data
- # 10 - Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac6515
- # 11 - Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac6514