Fonte: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. Unidade: IAG
Assuntos: ASTROBIOLOGIA, ASTROQUÍMICA
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CANELO, Carla Martinez et al. Variations in the 6.2 μm emission profile in starburst-dominated galaxies: a signature of polycyclic aromatic nitrogen heterocycles (PANHs)?. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v. 475, p. 3746-3763, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/stx3351. Acesso em: 23 abr. 2024.APA
Canelo, C. M., Friaça, A. C. S., Sales, D. A., Pastoriza, M. G., & Ruschel-Dutra, D. (2018). Variations in the 6.2 μm emission profile in starburst-dominated galaxies: a signature of polycyclic aromatic nitrogen heterocycles (PANHs)? MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 475, 3746-3763. doi:10.1093/mnras/stx3351NLM
Canelo CM, Friaça ACS, Sales DA, Pastoriza MG, Ruschel-Dutra D. Variations in the 6.2 μm emission profile in starburst-dominated galaxies: a signature of polycyclic aromatic nitrogen heterocycles (PANHs)? [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;475 3746-3763.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1093/mnras/stx3351Vancouver
Canelo CM, Friaça ACS, Sales DA, Pastoriza MG, Ruschel-Dutra D. Variations in the 6.2 μm emission profile in starburst-dominated galaxies: a signature of polycyclic aromatic nitrogen heterocycles (PANHs)? [Internet]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. 2018 ;475 3746-3763.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1093/mnras/stx3351
