Near-infrared observations of outflows and young stellar objects in the massive star-forming region AFGL 5180

Context. Massive stars play important roles throughout the universe; however, their formation remains poorly understood. Observations of jets and outflows in high-mass star-forming regions, as well as surveys of young stellar object (YSO) content, can help test theoretical models of massive star for...

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Detalles Bibliográficos
Autores: Crowe, S., Fedriani, R., Tan, J. C., Whittle, M., Zhang, Y., Caratti o Garatti, A., Farias, J. P., Gautam, A., Telkamp, Z., Rothberg, B., Grudić, M., Andersen, M., Cosentino, G., Garcia-Lopez, R., Rosero, V., Tanaka, K., Pinna, E., Rossi, F., Miller, D., Agapito, G., Plantet, C., Ghose, E., Christou, J., Power, J., Puglisi, A., Briguglio, R., Brusa, G., Taylor, G., Zhang, X., Mazzoni, T., Bonaglia, M., Esposito, S., Veillet, C.
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2024
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/370878
Acceso en línea:http://hdl.handle.net/10261/370878
Access Level:acceso abierto
Palabra clave:Techniques: high angular resolution
Stars: formation
Stars: individual: AFGL 5180
Stars: protostars
ISM: jets and outflows
Infrared: stars
Descripción
Sumario:Context. Massive stars play important roles throughout the universe; however, their formation remains poorly understood. Observations of jets and outflows in high-mass star-forming regions, as well as surveys of young stellar object (YSO) content, can help test theoretical models of massive star formation.