Galactic runaway O and Be stars found using Gaia DR3
[Context] A relevant fraction of massive stars are runaway stars. These stars move with a significant peculiar velocity with respect to their environment.
| Autores: | , , |
|---|---|
| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2023 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/352761 |
| Acceso en línea: | http://hdl.handle.net/10261/352761 |
| Access Level: | acceso abierto |
| Palabra clave: | Catalogs Stars: early-type Stars: kinematics and dynamics X-rays: binaries Stars: emission-line Gamma rays: stars |
| Sumario: | [Context] A relevant fraction of massive stars are runaway stars. These stars move with a significant peculiar velocity with respect to their environment. |
|---|