A self-consistent dynamical model of the Milky Way disc adjusted to Gaia data
[Context] Accurate astrometry achieved by Gaia for many stars in the Milky Way provides an opportunity to reanalyse the Galactic stellar populations from a large and homogeneous sample and to revisit the Galaxy gravitational potential.
| Autores: | , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2022 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/296515 |
| Acceso en línea: | http://hdl.handle.net/10261/296515 |
| Access Level: | acceso abierto |
| Palabra clave: | Galaxy: kinematics and dynamics Galaxy: structure Galaxy: evolution Galaxy: disk Galaxy: general Surveys |
| Sumario: | [Context] Accurate astrometry achieved by Gaia for many stars in the Milky Way provides an opportunity to reanalyse the Galactic stellar populations from a large and homogeneous sample and to revisit the Galaxy gravitational potential. |
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