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Computational Methods for Collisional Stellar Systems

Computational Methods for Collisional Stellar Systems

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2817224099

Computational Methods for Collisional Stellar Systems

About this item

Full title

Computational Methods for Collisional Stellar Systems

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2023-05

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

Dense star clusters are spectacular self-gravitating stellar systems in our Galaxy and across the Universe - in many respects. They populate disks and spheroids of galaxies as well as almost every galactic center. In massive elliptical galaxies nuclear clusters harbor supermassive black holes, which might influence the evolution of their host galax...

Alternative Titles

Full title

Computational Methods for Collisional Stellar Systems

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2817224099

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2817224099

Other Identifiers

E-ISSN

2331-8422

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