An observational correlation between magnetic field, angular momentum and fragmentation in the envelopes of Class 0 protostars?

Autor: Eric Keto, Qizhou Zhang, Shih-Ping Lai, Valeska Valdivia, Josep M. Girart, Anaëlle Maury, Victoria Cabedo-Soto, Patrick Hennebelle, M. Gaudel, Ramprasad Rao, Maud Galametz

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 644, pp.A47. ⟨10.1051/0004-6361/202038854⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, 2020, 644, pp.A47. ⟨10.1051/0004-6361/202038854⟩
Digital.CSIC. Repositorio Institucional del CSIC
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Aims. The main goal of the following analysis is to assess the potential role of magnetic fields in regulating the envelope rotation, the formation of disks and the fragmentation of Class 0 protostars in multiple systems. Methods. We use the Submilli

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66cc53a93522f2c43aa615bcb7808e5f
https://hal-cea.archives-ouvertes.fr/cea-03037158