AB Aur, a Rosetta stone for studies of planet formation III. Continuum observations at 2 and 7 mm
[Context]: Observational constraints on dust properties in protoplanetary disks are key to better understanding disk evolution, their dynamics, and the pathway to planet formation, but also surface chemistry, the main driver of chemical complexity.
| Autores: | , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/369489 |
| Acceso en línea: | http://hdl.handle.net/10261/369489 |
| Access Level: | acceso abierto |
| Palabra clave: | Protoplanetary disks Stars: pre-main sequence Stars: protostars Radio continuum: ISM Radio continuum: planetary systems Submillimeter: planetary systems |
| Sumario: | [Context]: Observational constraints on dust properties in protoplanetary disks are key to better understanding disk evolution, their dynamics, and the pathway to planet formation, but also surface chemistry, the main driver of chemical complexity. |
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