19 citations · 42 across the 5 of their papers we have counts for
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Variations in the 6.2 m polycyclic aromatic hydrocarbon band in Active Galactic Nuclei- and Starburst-dominated galaxies
Carla M. Canelo, Dinalva A. Sales, Vitor Avelaneda +3
Polycyclic aromatic hydrocarbons (PAHs) are fundamental to understanding the interstellar medium (ISM) of several astrophysical objects. Normally present in Starburst (SB) galaxies…
Polycyclic aromatic hydrocarbons and the ionized gas
A. Silva-Ribeiro, A. C. Krabbe, C. M. Canelo +4
We present a study for a sample of galaxies with active nuclei to characterize the main type of PAH molecules present in these objects and the local physical conditions of their ir…
Profile comparison of the 6-9 m polycyclic aromatic hydrocarbon bands in starburst-dominated galaxies
Carla M. Canelo, Dinalva A. Sales, Amâncio C. S. Friaça +2
Polycyclic aromatic hydrocarbons (PAHs) are of great astrochemical and astrobiological interest due to their potential to form prebiotic molecules. We analyse the 7.7 and 8.6 m…
Isocyanic acid (HNCO) in the Hot Molecular Core G331.512-0.103: Observations and Chemical Modelling
Carla M. Canelo, Leonardo Bronfman, Edgar Mendoza +5
Isocyanic acid (HNCO) is a simple molecule with a potential to form prebiotic and complex organic species. Using a spectral survey collected with the Atacama Pathfinder EXperiment…