Erosion of a dense molecular core by a strong outflow from a massive protostar
[Context] Molecular outflows from massive protostars can impact the interstellar medium in different ways, adding turbulence on different spatial scales, dragging material at supersonic velocities, producing shocks and heating, and physically impinging onto dense structures that may be harboring oth...
| 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:10261/389907 |
| Acceso en línea: | http://hdl.handle.net/10261/389907 http://arxiv.org/abs/2502.17786v1 |
| Access Level: | acceso abierto |
| Palabra clave: | ISM: clouds ISM: jets and outflows Stars: formation Stars: winds, outflows |
| Sumario: | [Context] Molecular outflows from massive protostars can impact the interstellar medium in different ways, adding turbulence on different spatial scales, dragging material at supersonic velocities, producing shocks and heating, and physically impinging onto dense structures that may be harboring other protostars. |
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