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Flujo molecular episódico en el muy joven cúmulo protostellar Serpens Sur
Adele L Plunkett1, Héctor G Arce1, Diego Mardones2
1Astronomy Department, Yale University, New Haven, Connecticut 06511, USA.
Nature
|November 6, 2015
Resumen
Las salidas protoestelares exhiben eventos de eyección de masa episódica, incluso en las primeras etapas de la formación estelar dentro de cúmulos densos. Esto proporciona una turbulencia crucial para regular la formación de estrellas en estos entornos.
Área de la Ciencia:
- * Astronomía y astrofísica
- * Formación y evolución de las estrellas
- * Los chorros y salidas protostellares
Sus antecedentes:
- * La acumulación de masa protostellar se acompaña de pérdida de masa a través de chorros o salidas.
- * Se observan eventos de eyección episódica en las fases protostellares de Clase 0 y Clase I.
- * El comportamiento de las salidas en densos cúmulos de formación estelar no se entiende bien.
Objetivo del estudio:
- * Investigar la naturaleza de las salidas impulsadas por la acreción de las protoestrellas jóvenes en un entorno agrupado.
- * Para determinar si los eventos de eyección episódica ocurren en las primeras etapas de la evolución protostellar dentro de los cúmulos.
- * Comprender el papel de los flujos de salida en la transferencia de impulso y energía en cúmulos protoestelares.
Principales métodos:
- * Observación de una joven protoestrella de clase 0 en el centro del cúmulo protostellar Serpens Sur.
- * Análisis de la emisión (12) C(16) O (J=2-1) para identificar las características de las expulsiones de flujo.
- * Examen de las emisiones de la envolvente de CO2 para estudiar la cinemática de la caída y la rotación.
Principales resultados:
- * Se encontraron pruebas inequívocas de eventos de eyección de flujo episódico de la protoestrella.
- * Se detectaron veintidós características de eyección de salida distintas, con la más reciente mostrando la velocidad más alta.
- * El flujo de salida forma lóbulos bipolares que se originan en el pico de emisión del continuo de 1 mm, y la envoltura circundante muestra la caída y la rotación.
Conclusiones:
- * El flujo episódico, impulsado por la acreción, comienza en las primeras fases de la evolución protostellar.
- * Los flujos de salida protoestelares pueden permanecer intactos y funcionar dentro de entornos densos y agrupados.
- * Es probable que estos flujos de salida desempeñen un papel importante en la conducción de la turbulencia a través de una transferencia de impulso eficiente en los grupos.
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