Radial and azimuthal gradients of the moving groups in Gaia DR3: The slow and fast bar degeneracy problem
[Contex] The structure and dynamics of the central bar of the Milky Way (MW) are still under debate whilst being fundamental ingredients for the evolution of our Galaxy. The recent Gaia DR3 offers an unprecedented detailed view of the 6D phase space of the MW, allowing for a better understanding of...
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/365849 |
| Acceso en línea: | http://hdl.handle.net/10261/365849 |
| Access Level: | acceso abierto |
| Palabra clave: | Methods: data analysis Galaxy: disk Galaxy: evolution Galaxy: kinematics and dynamics Galaxy: structure |
| Sumario: | [Contex] The structure and dynamics of the central bar of the Milky Way (MW) are still under debate whilst being fundamental ingredients for the evolution of our Galaxy. The recent Gaia DR3 offers an unprecedented detailed view of the 6D phase space of the MW, allowing for a better understanding of the complex imprints of the bar on the phase space. |
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