Magnetic threads and gravity: ALMA observations of the infrared dark cloud G14.225-0.506

[Context] In the star formation process, the interplay between gravity, turbulence, and magnetic fields is significant, with magnetic fields apparently serving a regulatory function by opposing gravitational collapse. Nonetheless, the extent to which magnetic fields are decisive relative to turbulen...

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Detalles Bibliográficos
Autores: Añez-López, N., Busquet, Gemma, Girart, Josep Miquel, Liu, Junhao, Zhang, Qizhou, Koch, Patrick M., Maury, Anaëlle, Liu, Hauyu Baobab, Li, Zhi-Yun, Qiu, Keping, Li, Shanghuo, Chen, Huei-Ru Vivien, Tang, Ya Wen, Lai, Shih-Ping, Rao, Ramprasad, Ho, Paul
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2026
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:dnet:digitalcsic_::835db17b5ce95c113c1f7672779d0e26
Acceso en línea:http://hdl.handle.net/10261/431546
https://api.elsevier.com/content/abstract/scopus_id/105033031757
Access Level:acceso abierto
Palabra clave:ISM: clouds
ISM: magnetic fields
Stars: formation
Stars: massive
Descripción
Sumario:[Context] In the star formation process, the interplay between gravity, turbulence, and magnetic fields is significant, with magnetic fields apparently serving a regulatory function by opposing gravitational collapse. Nonetheless, the extent to which magnetic fields are decisive relative to turbulence and gravity, as well as the specific environments and conditions involved, remains uncertain.

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