The 3D time evolution of the dust size distribution in protostellar envelopes
[Context] Dust plays a fundamental role during protostellar collapse and disk and planet formation. Recent observations suggest that efficient dust growth can begin early in the protostellar envelopes, potentially even before the formation of the disk. Three-dimensional models of protostellar evolut...
| Autores: | , , |
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| Formato: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2026 |
| País: | España |
| Recursos: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:dnet:digitalcsic_::0b83fbe350f974d01e41101ea0487d71 |
| Acesso em linha: | http://hdl.handle.net/10261/431663 |
| Access Level: | acceso abierto |
| Palavra-chave: | Methods: numerical Protoplanetary disks Stars: formation Stars: protostars Dust, extinction Evolution |
| Resumo: | [Context] Dust plays a fundamental role during protostellar collapse and disk and planet formation. Recent observations suggest that efficient dust growth can begin early in the protostellar envelopes, potentially even before the formation of the disk. Three-dimensional models of protostellar evolution that address multi-size dust growth, gas and dust dynamics, and magnetohydrodynamics (MHD) are required to characterize the dust evolution in the embedded stages of star formation. |
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