Gas-star segregation and the resilience of King-family clusters to gas expulsion: analysis code and data
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kz (code pays fourni par la source)
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kz (code pays fourni par la source)
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kz (code pays fourni par la source)
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kz (code pays fourni par la source)
Almat Akhmetali, Adilkhan Assilkhan, Mordecai‐Mark Mac Low, Nurzhan Ussipov et autres
We investigate the structural evolution of young star clusters forming within centrally concentrated molecular clouds. Our simulations use the Torch framework, which integrates the FLASH magnetohydrodynamics code with the AMUSE environment, enabling a self-consistent treatment of gas dynamics, star formation, stellar evolution, …
kz, cn, ca (code pays fourni par la source)
Adilkhan Assilkhan, Sabrina M. Appel, Bekdaulet Shukirgaliyev, Ernazar Abdikamalov et autres
Protostellar jets are one of the earliest forms of stellar feedback, but their impact on star formation and cluster assembly in centrally concentrated molecular clouds remains poorly understood. We study how protostellar jets affect the star formation efficiency, the temporal variability of …
Adilkhan Assilkhan, Sabrina M. Appel, Bekdaulet Shukirgaliyev, Ernazar Abdikamalov et autres
Protostellar jets are one of the earliest forms of stellar feedback, but their impact on star formation and cluster assembly in centrally concentrated molecular clouds remains poorly understood. We study how protostellar jets affect the star formation efficiency, the temporal variability of …
Almat Akhmetali, Adilkhan Assilkhan, Mordecai‐Mark Mac Low, Nurzhan Ussipov et autres
We investigate the structural evolution of young star clusters forming within centrally concentrated molecular clouds. Our simulations use the Torch framework, which integrates the FLASH magnetohydrodynamics code with the AMUSE environment, enabling a self-consistent treatment of gas dynamics, star formation, stellar evolution, …
kz, us, ca, cn (code pays fourni par la source)
Vahid Amiri, Francesco Flammini Dotti, Xiaoying Pang, A. W. H. Kamlah et autres
We want to understand how the combined effect of initial substructure, primordial mass segregation, and primordial binaries affects the dynamical evolution of the cluster, and which one of these features is the most important to agree with observations. Methods. We use Nbody6++GPU …
Vahid Amiri, Francesco Flammini Dotti, Xiaoying Pang, A. W. H. Kamlah et autres
We want to understand how the combined effect of initial substructure, primordial mass segregation, and primordial binaries affects the dynamical evolution of the cluster, and which one of these features is the most important to agree with observations. Methods. We use Nbody6++GPU …
de, ua, pl (code pays fourni par la source)
Adilkhan Assilkhan, Sabrina M. Appel, Bekdaulet Shukirgaliyev, Ernazar Abdikamalov et autres
This package provides the analysis products and raw simulation snapshots accompanying the paper "Centrally concentrated star formation in young clusters II: Jet feedback." It includes time‑history tables, per‑snapshot stellar particle catalogues, raw FLASH/Torch HDF5 snapshots at two reference epochs, and density‑slice movies …
Abylay Bissekenov, Xiaoying Pang, Rainer Spurzem, Bekdaulet Shukirgaliyev et autres
Abstract Wide (soft) binaries are expected to be rapidly disrupted in dense stellar environments, yet they are observed in both the Galactic field and open clusters (OCs). In this Letter, we investigate the formation and disruption of wide binaries in star clusters …
kz, cn, de, ua, pl (code pays fourni par la source)
Abylay Bissekenov, Xiaoying Pang, Rainer Spurzem, Bekdaulet Shukirgaliyev et autres
Wide (soft) binaries are expected to be rapidly disrupted in dense stellar environments, yet they are observed in both the Galactic field and open clusters (OCs). In this paper, we investigate the formation and disruption of wide binaries in star clusters using …
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