TheGaia-ESO Survey: Stellar content and elemental abundances in the massive cluster NGC 6705

2014/07/06 by T. Cantat-Gaudin, A. Vallenari, S. Zaggia +68 · 80 citations
Mathematics · Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Biology #Cluster (spacecraft) #Computer science #Content (measure theory) #Context (archaeology) #Geology #Globular cluster #Key (lock) #Mathematics #Open cluster #Paleontology #Physics #Stars #Stellar, planetary, and galactic studies #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201423851

published in Astronomy and Astrophysics 569, A17 (EDP Sciences)

arxiv created 2014/07/06 · openalex publication_date 2014/07/15 · arxiv updated 2014/09/10 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. Chemically inhomogeneous populations are observed in most globular clusters, but not in open clusters. Cluster mass seems to play a key role in the existence of multiple populations.

Citations

• Central energy equipartition in multimass models of globular clusters
• The Dartmouth Stellar Evolution Database
• The influence of multiple stars on the high-mass stellar initial mass function and age dating of young massive star clusters
• parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
• Abundance Variations within Globular Clusters
• DAOPHOT - A computer program for crowded-field stellar photometry
• Correcting for the Effects of Interstellar Extinction
• Multiple populations in globular clusters. Lessons learned from the Milky Way globular clusters

Cited by

• NGC 6535: the lowest mass Milky Way globular cluster with a Na-O anti-correlation?
• TheGaia-ESO Survey: double-, triple-, and quadruple-line spectroscopic binary candidates
• Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra
• OCCASO – II. Physical parameters and Fe abundances of red clump stars in 18 open clusters
• Double-lined spectroscopic binaries in M11