M. J. Cordero
Physics and Astronomy · Indiana University
Publications
22
Citations
596
Est. group size
—
Recurring co-author estimate
Active years
20
Publishing since 2006
M. J. Cordero studies stellar clusters, which are large groups of stars that formed together, and investigates whether these clusters contain multiple distinct populations of stars with different ages or chemical makeup. Much of the work focuses on clusters in the Magellanic Clouds, small galaxies neighboring our own Milky Way, using observations to test how a cluster's age and its stars' rotation shape what we observe.
Publication activity was concentrated around 2016-2019 and has been sparse since, with very few papers in the most recent years.
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- The search for multiple populations in Magellanic Cloud Clusters – III. No evidence for multiple populations in the SMC cluster NGC 419
Monthly Notices of the Royal Astronomical Society · 2017
- Age as a major factor in the onset of multiple populations in stellar clusters
Monthly Notices of the Royal Astronomical Society · 2017
- A young cluster with an extended main-sequence turnoff: confirmation of a prediction of the stellar rotation scenario
Monthly Notices of the Royal Astronomical Society Letters · 2016
- The search for multiple populations in Magellanic Cloud clusters – I. Two stellar populations in the Small Magellanic Cloud globular cluster NGC 121
Monthly Notices of the Royal Astronomical Society · 2016
- The search for multiple populations in Magellanic Cloud clusters – II. The detection of multiple populations in three intermediate-age SMC clusters
Monthly Notices of the Royal Astronomical Society · 2016
- Monthly Notices of the Royal Astronomical Society×5
- Monthly Notices of the Royal Astronomical Society Letters×1
- Revista Mexicana de Astronomía y Astrofísica×1
- Research Notes of the AAS×1
- yCat×1
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
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