Source: The Astrophysical Journal. Unidade: EACH
Subjects: MAGNETOHIDRODINÂMICA, MEIO INTERESTELAR
ABNT
JESUS, Lorena do Carmo et al. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, v. 905, n. 2, p. 01-12, 2020Tradução . . Disponível em: https://doi.org/10.3847/1538-4357/abc331. Acesso em: 11 nov. 2024.APA
Jesus, L. do C., González-Casanova, D. F., Falceta Gonçalves, D. A., Lazarian, A., Jablonski, F., Zhang, J. -F., et al. (2020). Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium. The Astrophysical Journal, 905( 2), 01-12. doi:10.3847/1538-4357/abc331NLM
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 11 ] Available from: https://doi.org/10.3847/1538-4357/abc331Vancouver
Jesus L do C, González-Casanova DF, Falceta Gonçalves DA, Lazarian A, Jablonski F, Zhang J-F, Ferreira IS, Castro MLD, Yang B. Synchrotron Intensity and Polarization Gradients: Tools to Obtain the Magnetization Level in a Turbulent Medium [Internet]. The Astrophysical Journal. 2020 ; 905( 2): 01-12.[citado 2024 nov. 11 ] Available from: https://doi.org/10.3847/1538-4357/abc331