Are the ONC, Pleiades, and Hyades snapshots of the same embedded cluster?

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Conflicts of Interest

Identified Weaknesses

Rating Explanation

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Paper Summary

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From Orion's Cradle to the Pleiades' Promenade: A Star Cluster's Journey Through Time

This study simulates the evolution of an Orion Nebula Cluster-like star cluster, finding that over time it loses mass and expands, potentially resembling the Pleiades in 100 million years and the Hyades in 700 million years. This suggests these clusters may represent different stages in the evolution of a similar initial star-forming region.

Possible Conflicts of Interest

None identified

Identified Weaknesses

Reliance on Simulations

The study heavily relies on simulations and theoretical models, and while these are valuable tools, they don't perfectly represent reality. There may be unknown factors influencing the evolution of star clusters that the models don't fully capture.

Uncertainties in Initial Conditions

The simulations rely on certain assumptions about initial conditions, and the actual initial conditions of these clusters are not perfectly known. Uncertainties in these parameters can impact the results of the simulations.

Rating Explanation

This is a well-conducted study using sophisticated N-body simulations to investigate a relevant astrophysical question. While it relies on simulations and certain assumptions, the study is thorough and insightful and contributes meaningfully to our understanding of star cluster evolution. The study acknowledges limitations and the results generally align with observational data. Thus, a rating of 4 is justified.

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