Fonte: Monthly Notices of the Royal Astronomical Society. Unidade: IAG
Assuntos: GALÁXIAS, GALÁXIAS ELÍPTICAS
ABNT
DANTAS, M. L. L e COELHO, Paula Rodrigues Teixeira e GONÇALVES, T S. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass?. Monthly Notices of the Royal Astronomical Society, v. 492, n. 2, p. 2996-3011, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/stz3609. Acesso em: 08 out. 2024.APA
Dantas, M. L. L., Coelho, P. R. T., & Gonçalves, T. S. (2020). UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? Monthly Notices of the Royal Astronomical Society, 492( 2), 2996-3011. doi:10.1093/mnras/stz3609NLM
Dantas MLL, Coelho PRT, Gonçalves TS. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 2): 2996-3011.[citado 2024 out. 08 ] Available from: https://doi.org/10.1093/mnras/stz3609Vancouver
Dantas MLL, Coelho PRT, Gonçalves TS. UV bright red-sequence galaxies: how do UV upturn systems evolve in redshift and stellar mass? [Internet]. Monthly Notices of the Royal Astronomical Society. 2020 ; 492( 2): 2996-3011.[citado 2024 out. 08 ] Available from: https://doi.org/10.1093/mnras/stz3609