Are the filaments formed by synchrotron thermal instability bright? (1993)
Source: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assunto: ASTRONOMIA
ABNT
GOUVEIA DAL PINO, Elisabete Maria de e OPHER, Reuven. Are the filaments formed by synchrotron thermal instability bright?. Monthly Notices of the Royal Astronomical Society, v. 263, n. 3, p. 687-694, 1993Tradução . . Disponível em: https://doi.org/10.1093/mnras/263.3.687. Acesso em: 27 nov. 2025.APA
Gouveia dal Pino, E. M. de, & Opher, R. (1993). Are the filaments formed by synchrotron thermal instability bright? Monthly Notices of the Royal Astronomical Society, 263( 3), 687-694. doi:10.1093/mnras/263.3.687NLM
Gouveia dal Pino EM de, Opher R. Are the filaments formed by synchrotron thermal instability bright? [Internet]. Monthly Notices of the Royal Astronomical Society. 1993 ; 263( 3): 687-694.[citado 2025 nov. 27 ] Available from: https://doi.org/10.1093/mnras/263.3.687Vancouver
Gouveia dal Pino EM de, Opher R. Are the filaments formed by synchrotron thermal instability bright? [Internet]. Monthly Notices of the Royal Astronomical Society. 1993 ; 263( 3): 687-694.[citado 2025 nov. 27 ] Available from: https://doi.org/10.1093/mnras/263.3.687
