KRATOS: A large suite of N-body simulations to interpret the stellar kinematics of LMC-like discs
The Large and Small Magellanic Cloud (LMC and SMC, respectively) are the brightest satellites of the Milky Way (MW) and, for the previous thousands of million years, they have been interacting with one another. Since observations only provide a static picture of the entire process, numerical simulat...
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| Tipo de recurso: | conjunto de datos |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consorci de Serveis Universitaris de Catalunya (CSUC) |
| Repositorio: | CORA.Repositori de Dades de Recerca |
| OAI Identifier: | oai:dnet:cora.rdr____::c90614433e17578dd2e5449a40015169 |
| Acceso en línea: | https://doi.org/10.34810/DATA1156 |
| Access Level: | acceso abierto |
| Palabra clave: | Astronomy and Astrophysics Astronomy Astrophysics Simulations Galaxies Magellanic Clouds KRATOS Large Magellanic Cloud Small Magellanic Cloud Milky Way LMC SMC MW |
| Sumario: | The Large and Small Magellanic Cloud (LMC and SMC, respectively) are the brightest satellites of the Milky Way (MW) and, for the previous thousands of million years, they have been interacting with one another. Since 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. KRATOS is a comprehensive suite of 28 open access pure N-body simulations of isolated and interacting LMC-like galaxies, to study the formation of substructures in their disc after the interaction with an SMC-mass galaxy. |
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