Research Progress in Star Clusters and Stellar Systems
A special issue of Galaxies (ISSN 2075-4434).
Deadline for manuscript submissions: closed (30 November 2023) | Viewed by 1099
Special Issue Editor
2. Argelander-Institut für Astronomie (AIfA), Auf dem Hügel 71, D-53121 Bonn, Germany
Interests: stellar dynamics; N-body simulations; gravitational waves; astrophysics of black holes; star formation
Special Issue Information
Dear Colleagues,
Star clusters are the building blocks of our luminous Universe. By virtue of over-density and random motion of stars, gravitationally bound star clusters and stellar associations can give rise to a wide range of astrophysical phenomena such as the formation of unusual stellar collision products, compact-object binaries, and gravitational-wave sources. How very dense, young star clusters are assembled, especially those containing hundred-thousands to millions of young stars within some parsecs, is still largely an open question. Undoubtedly, star clusters and stellar systems offer a wide, rich, and multi-disciplinary field of research, equivocally for observers and theorists. With present and upcoming cutting-age observatories such as Very Large Telescope, Gaia, James Webb Space Telescope, Thirty Meter Telescope, Athena, third-generation and space-based gravitational-wave detectors and with the continued developments of high-performance computing, the research field of stellar systems and star clusters will only escalate and broaden.
This Special Issue, hosted by Galaxies, aims at bringing together star cluster-related topics that are of particular interest at present or in the near future. We invite submissions of both original research papers and review-style articles related to star clusters and stellar systems (young clusters, open clusters, stellar associations, gas-embedded systems, globular clusters, galactic nuclear clusters). We are happy to consider all topics concerning star clusters and especially encourage submissions covering one or more of the following sub-topics:
- Formation and assembly of young star clusters;
- Physics of dynamical systems;
- Computational challenges of gravitational many-body systems;
- Stellar remnants in star clusters: observational signatures;
- Dynamical assembly of gravitational-wave sources;
- Open star clusters;
- Stellar initial mass function;
- Intermediate mass black holes in star clusters;
- Observing stellar clusters and streams with Gaia;
- Prospects of observing clusters with next-generation telescopes;
- Applications of data science and machine learning to stellar systems.
Dr. Sambaran Banerjee
Guest Editor
Manuscript Submission Information
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Keywords
- globular clusters
- open clusters and associations
- black holes
- gravitational-wave sources
- astrometry and photometry
- many-body systems
- N-body simulation
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