Formation of star clusters with extended main-sequence turn-offs in the Magellanic Clouds: the origin of young stellar objects in older clusters
Author:
Affiliation:
1. International Centre for Radio Astronomy Research/The University of Western Australia, M468, 35 Stirling Hwy, Crawley, WA 6009, USA
2. ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), Australia
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/481/3/3651/25838528/sty2445.pdf
Reference65 articles.
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4. Formation of Star Clusters in the Large Magellanic Cloud and Small Magellanic Cloud. I. Preliminary Results on Cluster Formation from Colliding Gas Clouds
5. Formation and evolution of the Magellanic Clouds - I. Origin of structural, kinematic and chemical properties of the Large Magellanic Cloud
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1. Star cluster formation from giant molecular clouds in the small magellanic cloud about 2 Gyr ago: their origin, structures, and kinematics;Monthly Notices of the Royal Astronomical Society;2021-12-22
2. Simulations of globular clusters within their parent galaxies: multiple stellar populations and internal kinematics;Monthly Notices of the Royal Astronomical Society;2020-10-31
3. Star formation from non-turbulent gas within globular clusters: discrete multiple bursts and top-light mass functions;Monthly Notices of the Royal Astronomical Society;2019-04-16
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