Surface brightness profile of the Milky Way’s nuclear star cluster
[Context] Although the Milky Way nuclear star cluster (MWNSC) was discovered more than four decades ago, several of its key properties have not been determined unambiguously up to now because of the strong and spatially highly variable interstellar extinction toward the Galactic centre.
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2014 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/98521 |
| Acceso en línea: | http://hdl.handle.net/10261/98521 |
| Access Level: | acceso abierto |
| Palabra clave: | Dust Extinction Galaxy: center Galaxy: nucleus Galaxy: structure Galaxies: nuclei Infrared: stars |
| Sumario: | [Context] Although the Milky Way nuclear star cluster (MWNSC) was discovered more than four decades ago, several of its key properties have not been determined unambiguously up to now because of the strong and spatially highly variable interstellar extinction toward the Galactic centre. |
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