arXiv (All)
open access
Towards breaking the degeneracy between stellar ages and unresolved multiplicity
Stellar age is the central desirable parameter we need to disentangle different Galactic formation scenarios. Nevertheless, no stellar age dating method is completely model-independent. Even in the best-case scenarios, present-day stellar age estimates are only precise to $\sim7\%$ and accurate to $
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Growth from KiDS: Stellar mass assembly of galaxies since z=2 in the light of Kilo-Degree Survey#1049117
- The DESI DR1 peculiar velocity survey: Growth rate measurements from the galaxy power spectrum#642091
- NOCTURNE. II. Extreme radio variability in the heart of early-stage active galactic nuclei#1110745
- Weighing Galaxies Inside-Out: Small-Scale Lensing and the Stellar Mass Problem#1156813
- Distinct Population of Wolf-Rayet Stars in the Low-Metallicity Galaxy NGC 6822. Quantitative analysis of optical and UV spectra of the complete sample#1037601
Record · ID 1145074
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive