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Spectroscopic Constraints on the Mid-infrared Attenuation Curve. I. Attenuation Model Using Polycyclic Aromatic Hydrocarbon Emission

We introduce a novel model to spectroscopically constrain the mid-infrared (MIR) extinction/attenuation curve from 3–17 μ m, using polycyclic aromatic hydrocarbon (PAH) emission drawn from an AKARI–Spitzer extragalactic cross-archival data set. Currently proposed MIR extinction curves vary significa...

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Bibliografische gegevens
Hoofdauteurs: Thomas S.-Y. Lai, J. D. T. Smith, Els Peeters, Henrik W. W. Spoon, Shunsuke Baba, Masatoshi Imanishi, Takao Nakagawa
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
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Online toegang:https://doi.org/10.3847/1538-4357/ad354b
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