A multi-frequency, multi-epoch radio continuum study of the Quintuplet cluster with the Very Large Array
Context. The Quintuplet cluster, located in the Galactic Centre, is one of the few young massive clusters in the Milky Way. It allows us to study dozens of massive, post main-sequence stars individually, providing unique insights into the properties of the most massive stars.
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2025 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:dnet:digitalcsic_::ef9cae497f6f1fb1a931ba24030cc5ae |
| Acceso en línea: | http://hdl.handle.net/10261/429148 |
| Access Level: | acceso abierto |
| Palabra clave: | Stars: massive Galaxy: center Radio continuum: stars |
| Sumario: | Context. The Quintuplet cluster, located in the Galactic Centre, is one of the few young massive clusters in the Milky Way. It allows us to study dozens of massive, post main-sequence stars individually, providing unique insights into the properties of the most massive stars. |
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