A power spectral study of PHANGS galaxies with JWST MIRI: On the spatial scales of dust and PAHs

Abstract

The interstellar medium (ISM) consists of a diversity of structures across a range of spatial scales, intimately tied to galactic evolution. In this work, Fourier analysis is used to characterize the spatial structures of dust and Polycyclic Aromatic Hydrocarbons (PAHs) in the ISM of PHANGS-JWST galaxies, observed in the four photometric mid-infrared (MIR) filters from F770W to F2100W (i.e., 7.7 to 21$\mu$m)). We quantify the abundance of structure on different spatial scales using the power-law slope, $\alpha$, of the spatial power spectra. The distribution of $\alpha$ across all length scales differs significantly between filters, with steeper slopes for PAH-dominated filters (${\alpha }_{F770W}=2.19_{-0.15}^{+0.16}$, ${\alpha }_{F1130W}=1.88_{-0.37}^{+0.25}$) and shallower for the dust-continuum (${\alpha }_{F1000W}=1.48_{-0.47}^{+0.33}$, ${\alpha }_{F2100W}=0.94_{-0.28}^{+0.23}$). The distribution of $\alpha$ across galaxies is narrower for PAH-dominated than for thermal dust-dominated bands, highlighting that PAHs trace photo-dissociation regions dominated by similar physical processes, whereas dust structures are an integrated property over the diverse evolutionary histories of their host galaxies. Unlike dust structures, PAH-sensitive bands display a break in the power spectrum: below a characteristic scale, ${\ell }_0=160{\mathrm{pc}}_{-50\mathrm{pc}}^{+110\mathrm{pc}}$, PAH structures are suppressed.

13 pages, 8 figured. ApJ in press

References in corpus (11)

• The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium
• The PHANGS-HST Survey: Physics at High Angular resolution in Nearby GalaxieS with the Hubble Space Telescope
• The PHANGS-JWST Treasury Survey: Star Formation, Feedback, and Dust Physics at High Angular resolution in Nearby GalaxieS
• Star formation scaling relations at ~100 pc from PHANGS: Impact of completeness and spatial scale
• Turbulence in the Interstellar Medium
• Turbulence from localized random expansion waves
• Core Mass Function: The Role of Gravity
• PHANGS-JWST First Results: Mid-infrared emission traces both gas column density and heating at 100 pc scales
• PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA
• The structure and characteristic scales of molecular clouds
• The Interstellar Medium: The Key Component in Galactic Evolution and Modern Cosmology

Cited by in corpus (1)

• Aromatic Species in the Molecular Universe