Extended main sequence turnoffs in open clusters as seen by Gaia – I. NGC 2818 and the role of stellar rotation

Author:

Bastian N1,Kamann S1ORCID,Cabrera-Ziri I2,Georgy C3,Ekström S3,Charbonnel C34,de Juan Ovelar M1,Usher C1ORCID

Affiliation:

1. Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK

2. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

3. Department of Astronomy, University of Geneva, Chemin des Maillettes 51, CH-1290, Versoix, Switzerland

4. IRAP, UMR 5277, CNRS and Université de Toulouse, 14, avenue douard Belin, F-31400 Toulouse, France

Funder

European Research Council

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 57 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Extended main sequences in star clusters;Fundamental Research;2024-01

2. UOCS-XII. A study of open cluster NGC 6940 using UVIT/AstroSat cluster properties and exotic populations;Monthly Notices of the Royal Astronomical Society;2023-12-18

3. Exploring the origin of the extended main-sequence turn-off in M37 through the white dwarf cooling sequence;Monthly Notices of the Royal Astronomical Society;2023-06-22

4. The broadening of the main sequence in the open cluster M38;Monthly Notices of the Royal Astronomical Society;2023-06-20

5. On the Origin of the Split Main Sequences of the Young Massive Cluster NGC 1856;The Astrophysical Journal;2023-05-30

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