Rodriguez, Facundo 
; Montero-Dorta, Antonio D. ; Angulo, Raul E. ; Artale, María Celeste ; Merchán, Manuel
Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IF
Assuntos: COSMOLOGIA, GALÁXIAS, ESTRUTURA DO UNIVERSO, MÉTODOS NUMÉRICOS
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RODRIGUEZ, Facundo et al. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies. Monthly Notices of the Royal Astronomical Society, v. 505, n. 3, p. 3192-3205, 2021Tradução . . Disponível em: https://doi.org/10.1093/mnras/stab1571. Acesso em: 08 out. 2025.APA
Rodriguez, F., Montero-Dorta, A. D., Angulo, R. E., Artale, M. C., & Merchán, M. (2021). The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies. Monthly Notices of the Royal Astronomical Society, 505( 3), 3192-3205. doi:10.1093/mnras/stab1571NLM
Rodriguez F, Montero-Dorta AD, Angulo RE, Artale MC, Merchán M. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 505( 3): 3192-3205.[citado 2025 out. 08 ] Available from: https://doi.org/10.1093/mnras/stab1571Vancouver
Rodriguez F, Montero-Dorta AD, Angulo RE, Artale MC, Merchán M. The galaxy size–halo mass scaling relations and clustering properties of central and satellite galaxies [Internet]. Monthly Notices of the Royal Astronomical Society. 2021 ; 505( 3): 3192-3205.[citado 2025 out. 08 ] Available from: https://doi.org/10.1093/mnras/stab1571
