30 Doradus, the double stellar birth scenario by $N$-body \& \textsc{warpfield} clouds
R. Dom\'inguez, Eric W. Pellegrini, Ralf S. Klessen, Daniel Rahner

TL;DR
This study models the formation and evolution of 30 Doradus's stellar populations using N-body simulations and cloud evolution code, supporting a double star formation scenario with a re-collapse process.
Contribution
It introduces a combined N-body and cloud evolution modeling approach to reproduce the observed multiple stellar generations in 30 Doradus.
Findings
Models reproduce observed stellar ages and spatial distributions.
Second-generation stars are more concentrated than first-generation.
Results support a re-collapse origin for multiple stellar populations.
Abstract
We study the evolution of embedded star clusters as possible progenitors to reproduce 30 Doradus, specifically the compact star cluster known as R136 and its surrounding stellar family, which is believed to be part of an earlier star formation event. We employ the high-precision stellar dynamics code NBODY6++GPU to calculate the dynamics of the stars embedded in different evolving molecular clouds modelled by the 1D cloud/clusters evolution code WARPFIELD. We explore clouds with initial masses of M that (re)-collapse allowing for the birth of a second generation of stars. We explore different star formation efficiencies in order to find the best set of parameters that can reproduce the observation measurements. Our best-fit models correspond to a first stellar generation with masses between - M and…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
