Jensen, J. J; Honig, S. F; Rakshit, S; Alonso-Herrero, A; Asmus, D; Gandhi, P; Kishimoto, M; Smette, A; Tristram, K. R. W
(Oxford University Press on behalf of the Royal Astronomical Society, 2017-08)
Spectral features from polycyclic aromatic hydrocarbon (PAH) molecules observed in the
mid-infrared (mid-IR) range are typically used to infer the amount of recent and ongoing star
formation on kiloparsec scales around ...