Four stellar populations and extreme helium variation in the massive outer-halo globular cluster NGC 2419
Author:
Affiliation:
1. Dipartimento di Fisica e Astronomia ‘Galileo Galilei’, Univ. di Padova, Vicolo dell’Osservatorio 3, Padova I-35122, Italy
2. Centro di Ateneo di Studi e Attivita’ Spaziali ‘Giuseppe Colombo’ – CISAS, Via Venezia 15, Padova I-35131, Italy
Funder
European Research Council
Horizon 2020
Marie Sklodowska-Curie
Ministero dell'Istruzione, dell'Università e della Ricerca
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1477/28753239/stz1477.pdf
Reference73 articles.
1. THE ACS SURVEY OF GLOBULAR CLUSTERS. V. GENERATING A COMPREHENSIVE STAR CATALOG FOR EACH CLUSTER
2. Early disc accretion as the origin of abundance anomalies in globular clusters
3. Mean proper motions, space orbits, and velocity dispersion profiles of Galactic globular clusters derived fromGaiaDR2 data
4. Evidence for multiple populations in the massive globular cluster NGC 2419 from deep uVI LBT photometry★
5. Transforming observational data and theoretical isochrones into the ACS/WFC Vega-mag system
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