Source: Monthly Notices Royal Astronomical Society - MNRAS. Unidade: IQSC
Assunto: ASTROQUÍMICA
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VICHIETTI, Rafael Mario et al. Implications of the (H2O)n + CO↔trans-HCOOH + (H2O)n–1 (n = 1, 2, and 3) reactions for primordial atmospheres of Venus and Earth. Monthly Notices Royal Astronomical Society - MNRAS, v. 475, p. 3191–3200, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx3368. Acesso em: 19 out. 2024.APA
Vichietti, R. M., Spada, R. F. K., Silva, A. B. F. da, Machado, F. B. C., & Haiduke, R. L. A. (2018). Implications of the (H2O)n + CO↔trans-HCOOH + (H2O)n–1 (n = 1, 2, and 3) reactions for primordial atmospheres of Venus and Earth. Monthly Notices Royal Astronomical Society - MNRAS, 475, 3191–3200. doi:10.1093/mnras/stx3368NLM
Vichietti RM, Spada RFK, Silva ABF da, Machado FBC, Haiduke RLA. Implications of the (H2O)n + CO↔trans-HCOOH + (H2O)n–1 (n = 1, 2, and 3) reactions for primordial atmospheres of Venus and Earth [Internet]. Monthly Notices Royal Astronomical Society - MNRAS. 2018 ; 475 3191–3200.[citado 2024 out. 19 ] Available from: https://doi.org/10.1093/mnras/stx3368Vancouver
Vichietti RM, Spada RFK, Silva ABF da, Machado FBC, Haiduke RLA. Implications of the (H2O)n + CO↔trans-HCOOH + (H2O)n–1 (n = 1, 2, and 3) reactions for primordial atmospheres of Venus and Earth [Internet]. Monthly Notices Royal Astronomical Society - MNRAS. 2018 ; 475 3191–3200.[citado 2024 out. 19 ] Available from: https://doi.org/10.1093/mnras/stx3368