paper

A panchromatic spatially-resolved analysis of nearby galaxies -- I. Sub-kpc scale Main Sequence in grand-design spirals

arXiv:2001.04479 · doi:10.1093/mnras/staa433

Abstract

We analyse the spatially resolved relation between stellar mass (M) and star formation rate (SFR) in disk galaxies (i.e. the Main Sequence, MS). The studied sample includes eight nearby face-on grand-design spirals, e.g. the descendant of high-redshift, rotationally-supported star-forming galaxies. We exploit photometric information over 23 bands, from the UV to the far-IR, from the publicly available DustPedia database to build spatially resolved maps of stellar mass and star formation rates on sub-galactic scales of 0.5-1.5 kpc, by performing a spectral energy distribution fitting procedure that accounts for both the observed and the obscured star formation processes, over a wide range of internal galaxy environments (bulges, spiral arms, outskirts). With more than 30 thousands physical cells, we have derived a definition of the local spatially resolved MS per unit area for disks, =0.82log-8.69. This is consistent with the bulk of recent results based on optical IFU, using the H line emission as a SFR tracer. Our work extends the analysis at lower sensitivities in both M and SFR surface densities, up to a factor 10. The self consistency of the MS relation over different spatial scales, from sub-galactic to galactic, as well as with a rescaled correlation obtained for high redshift galaxies, clearly proves its universality.

arXiv comment21 pages, 15 figures. Accepted for publication in MNRAS

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