ALMA-IMF: IV. A comparative study of the main hot cores in W43-MM1: Detection, temperature, and molecular composition
[Context] Hot cores are signposts of the protostellar activity of dense cores in star-forming regions. W43-MM1 is a young region that is very rich in terms of high-mass star formation, which is highlighted by the presence of large numbers of high-mass cores and outflows.
| Autores: | , , , , , , , , , , , , , , , , , , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2022 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/296448 |
| Acceso en línea: | http://hdl.handle.net/10261/296448 |
| Access Level: | acceso abierto |
| Palabra clave: | Stars: formation Stars: massive ISM: abundances ISM: molecules Radio lines: ISM |
| Sumario: | [Context] Hot cores are signposts of the protostellar activity of dense cores in star-forming regions. W43-MM1 is a young region that is very rich in terms of high-mass star formation, which is highlighted by the presence of large numbers of high-mass cores and outflows. |
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