Dissecting the disk and the jet of a massive (proto)star: an ALMA view of IRAS 20126+4104
[Context] The study of disks around early-type (proto)stars has recently been boosted by a new generation of instruments, and additional evidence has been found of disk+jet systems around stars of up to ∼20 M⊙. These results appear to confirm theoretical predictions that even 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:digital.csic.es:10261/385385 |
| Acceso en línea: | http://hdl.handle.net/10261/385385 https://api.elsevier.com/content/abstract/scopus_id/85215385453 |
| Access Level: | acceso abierto |
| Palabra clave: | Accretion, accretion disks ISM: jets and outflows Stars: formation Stars: massive |
| Sumario: | [Context] The study of disks around early-type (proto)stars has recently been boosted by a new generation of instruments, and additional evidence has been found of disk+jet systems around stars of up to ∼20 M⊙. These results appear to confirm theoretical predictions that even the most massive stars may form though disk-mediated accretion. |
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