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Published in 2019 at "Nature Astronomy"
DOI: 10.1038/s41550-019-0909-6
Abstract: Globular clusters (GCs) are thought to be ancient relics from the early formative phase of galaxies, although their physical origin remains uncertain 1 , 2 . GCs are most numerous around massive elliptical galaxies, where…
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Keywords:
star clusters;
elliptical galaxy;
giant elliptical;
globular clusters ... See more keywords
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Published in 2024 at "Nature Astronomy"
DOI: 10.1038/s41550-023-02168-6
Abstract: Cosmic rays (CR) are energetic nuclei that permeate the entire Galactic disk. Their existence requires the presence of powerful particle accelerators. While Galactic supernova explosions may supply the required energy, there is growing evidence that…
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Keywords:
cosmic ray;
winds star;
energy;
contribution winds ... See more keywords
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Published in 2025 at "Publications of the Astronomical Society of the Pacific"
DOI: 10.1088/1538-3873/adf00e
Abstract: This study investigates the identification X-ray binary systems (XRBs) and their association with nearby compact star clusters in the galaxies NGC 2403, NGC 4303, and NGC 1672. Using data from the Hubble Space Telescope (HST)/ACS/Wide…
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Keywords:
ngc 4303;
ngc 1672;
compact star;
star clusters ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa2425
Abstract: We provide a homogeneous set of structural parameters of 83 star clusters located at the periphery of the Small Magellanic Cloud (SMC) and the Large Magellanic Cloud (LMC). The clusters' stellar density and surface brightness…
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Keywords:
inner clusters;
viscacha survey;
lmc clusters;
star clusters ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa3493
Abstract: As the sensitivity of gravitational wave (GW) instruments improves and new networks start operating, hundreds of merging stellar-mass black holes (SBHs) and intermediate-mass black holes (IMBHs) are expected to be observed in the next few…
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Keywords:
black hole;
star clusters;
mass;
disruption events ... See more keywords
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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa444
Abstract: The coalescence of supermassive black holes (SMBHs) should generate the strongest sources of gravitational waves (GWs) in the Universe. However, the dynamics of their coalescence is the subject of much debate. In this study, we…
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Keywords:
supermassive black;
nuclear star;
mass;
accelerated orbital ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab1931
Abstract: Recent observations of young embedded clumpy clusters and statistical identifications of binary star clusters have provided new insights into the formation process and subsequent dynamical evolution of star clusters. The early dynamical evolution of clumpy…
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Keywords:
milky way;
formation;
binary star;
star clusters ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab1968
Abstract: We investigate the evolutionary nexus between the morphology and internal kinematics of the central regions of collisional, rotating, multimass stellar systems, with special attention to the spatial characterization of the process of mass segregation. We…
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Keywords:
central dynamics;
dynamics multimass;
multimass rotating;
star clusters ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2238
Abstract: Most of massive stars form in binary or higher order systems in clumpy, substructured clusters. In the very first phases of their life, these stars are expected to interact with the surrounding environment, before being…
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Keywords:
impact binaries;
evolution;
evolution star;
clusters turbulent ... See more keywords
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Published in 2021 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stab2413
Abstract: We use the angular two-point correlation function (TPCF) to investigate the hierarchical distribution of young star clusters in 12 local (3–18 Mpc) star-forming galaxies using star cluster catalogs obtained with the Hubble Space Telescope (HST)…
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Keywords:
distribution;
hierarchical distribution;
star clusters;
environment ... See more keywords
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Published in 2022 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/stad1092
Abstract: Using radiation-hydrodynamic cosmological simulations, we present a detailed (0.1 pc resolution), physically motivated portrait of a typical-mass dwarf galaxy before the epoch of reionization, resolving the formation and evolution of star clusters into individual $10\:\mathrm{{\rm M}_{\odot…
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Keywords:
star;
star cluster;
star clusters;
formation ... See more keywords