KRATOS: A large suite of N -body simulations to interpret the stellar kinematics of LMC-like discs
[Context] The Large and Small Magellanic Clouds (LMC and SMC, respectively) are the brightest satellites of the Milky Way (MW), and for the last thousand million years they have been interacting with one another. As observations only provide a static picture of the entire process, numerical simulati...
| Autores: | , , , , , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/384245 |
| Acesso em linha: | http://hdl.handle.net/10261/384245 https://api.elsevier.com/content/abstract/scopus_id/85200333699 |
| Access Level: | acceso abierto |
| Palavra-chave: | Galaxies: interactions Galaxies: kinematics and dynamics Galaxies: structure Magellanic Clouds |
| Resumo: | [Context] The Large and Small Magellanic Clouds (LMC and SMC, respectively) are the brightest satellites of the Milky Way (MW), and for the last thousand million years they have been interacting with one another. As observations only provide a static picture of the entire process, numerical simulations are used to interpret the present-day observational properties of these kinds of systems, and most of them have been focused on attempting to recreate the neutral gas distribution and characteristics through hydrodynamical simulations. |
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