A revised age greater than 50 Myr for the young cluster IC 4665
Author:
Affiliation:
1. Astrophysics Group, Keele University , Keele, Staffordshire ST5 5BG , UK
2. MIT Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology , Cambridge, MA 02139 , USA
Abstract
Funder
European Space Agency
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad2845/51667972/stad2845.pdf
Reference58 articles.
1. New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
2. The Lithium-Depletion Boundary and the Age of the Young Open Cluster IC 2391
3. Spectroscopy of Very Low Mass Stars and Brown Dwarfs in IC 2391: Lithium Depletion and Hα Emission
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2. Correction to: a revised age greater than 50 Myr for the young cluster IC 4665;Monthly Notices of the Royal Astronomical Society;2024-04-25
3. Some Old Globular Clusters (and Stars) Inferring That the Universe Is Older Than Commonly Accepted;American Journal of Astronomy and Astrophysics;2024-04-11
4. Testing CCC+TL Cosmology with Observed Baryon Acoustic Oscillation Features;The Astrophysical Journal;2024-03-01
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