Main parameters relative to the SED decomposition.
|⟨ U ⟩||1.8||757||[2.2 × 10-5W m-2]|
Notes. ⟨ U ⟩ is the luminosity averaged starlight intensity; Teff ≃ ⟨ U ⟩ 1/6 × 17.5 K is the corresponding effective temperature of the grains; fPAH is the PAH-to-total-dust mass fraction; φ = LSF/(LISM + LSF) is the luminosity fraction of the star-forming component. is the effective dust temperature corresponding to the peak of the far-IR bump using Wien’s law.
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