Macedo, M., Wuensche, C. A., & Miranda, O. D. (2026). On the relative CNO underabundance in quasar absorption systems at $z \sim 3$ arising from Population III enrichment and attenuation by intermediate-mass black holes and primordial baryon accretion.
Cita Chicago Style (17a ed.)Macedo, Murilo, Carlos Alexandre Wuensche, y Oswaldo Duarte Miranda. On the Relative CNO Underabundance in Quasar Absorption Systems at $z \sim 3$ Arising from Population III Enrichment and Attenuation by Intermediate-mass Black Holes and Primordial Baryon Accretion. 2026.
Cita MLA (9a ed.)Macedo, Murilo, et al. On the Relative CNO Underabundance in Quasar Absorption Systems at $z \sim 3$ Arising from Population III Enrichment and Attenuation by Intermediate-mass Black Holes and Primordial Baryon Accretion. 2026.