HADES RV programme with HARPS-N at TNG: XII. The abundance signature of M dwarf stars with planets
[Context] Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing.
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/232773 |
| Acceso en línea: | http://hdl.handle.net/10261/232773 |
| Access Level: | acceso abierto |
| Palabra clave: | Planetary systems Stars: abundances Stars: late-type Techniques: spectroscopic |
| Sumario: | [Context] Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing. |
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