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The Not So Simple Stellar System ω Cen. II. Evidence in Support of a Merging Scenario
Annalisa Calamida, Alice Zocchi, Giuseppe Bono, Ivan Ferraro, Alessandra Mastrobuono-Battisti, Abhijit Saha, Giacinto Iannicola, Armin Rest, Giovanni Strampelli and Alfredo Zenteno The Astrophysical Journal 891(2) 167 (2020) https://doi.org/10.3847/1538-4357/ab77c0
The Not So Simple Globular Cluster ω Cen. I. Spatial Distribution of the Multiple Stellar Populations∗
A. Calamida, G. Strampelli, A. Rest, G. Bono, I. Ferraro, A. Saha, G. Iannicola, D. Scolnic, D. James, C. Smith and A. Zenteno The Astronomical Journal 153(4) 175 (2017) https://doi.org/10.3847/1538-3881/aa6397
HIGHLIGHTS OF COMMISSION 37 SCIENCE RESULTS
Giovanni Carraro, Richard de Grijs, Bruce Elmegreen, et al. Proceedings of the International Astronomical Union 11(T29A) 502 (2015) https://doi.org/10.1017/S174392131600096X
NUCLEOSYNTHESIS IN HELIUM-ENRICHED ASYMPTOTIC GIANT BRANCH MODELS: IMPLICATIONS FOR HEAVY ELEMENT ENRICHMENT IN ω CENTAURI
FROM THE COLOR-MAGNITUDE DIAGRAM OF ω CENTAURI AND (SUPER-)ASYMPTOTIC GIANT BRANCH STELLAR MODELS TO A GALACTIC PLANE PASSAGE GAS PURGING CHEMICAL EVOLUTION SCENARIO
Jacco Th. van Loon Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 368(1913) 801 (2010) https://doi.org/10.1098/rsta.2009.0259
CHEMICAL ABUNDANCES FOR 855 GIANTS IN THE GLOBULAR CLUSTER OMEGA CENTAURI (NGC 5139)
Lithium in a metal-poor external galaxy: ω Centauri
P. Bonifacio, L. Monaco, L. Sbordone, S. Villanova and E. Pancino Proceedings of the International Astronomical Union 5(S268) 269 (2009) https://doi.org/10.1017/S1743921310004230
Testing the AGB scenario as the origin of the extreme-helium population in ω Centauri
Fe and Al Abundances for 180 Red Giants in the Globular Cluster Omega Centauri (NGC 5139)
Christian I. Johnson, Catherine A. Pilachowski, Jennifer Simmerer and Dustin Schwenk The Astrophysical Journal 681(2) 1505 (2008) https://doi.org/10.1086/588634
From star clusters to dwarf galaxies: the properties of dynamically hot stellar systems