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We investigate several panchromatic scaling relations (SRs) for the dwarfirregular galaxy NGC 1569 using IFU data from the Metal-THINGS Survey. Amongthe spatially resolved properties analyzed, we explore SRs between the stellarmass, SFR, molecular gas, total gas, baryonic mass, gas metallicity, gasfraction, SFE and effective oxygen yields. Such multiwavelength SRs areanalyzed at a spatial resolution of 180 pc, by combining our IFU observationswith data from the surveys THINGS, CARMA, and archival data from DustPedia.Although we recover several known relations, our slopes are different topreviously reported ones. Our star formation main sequence, Kennicutt-Schmidt(KS) and molecular KS relations show higher SFRs, lower scatter, and highercorrelations, with steeper (1.21), and flatter slopes (0.96, 0.58)respectively. The shape of the SRs including metallicity, stellar mass, and gasfraction are flat, with an average value of 12+log(O/H) $\sim$ 8.12 dex. Thebaryonic mass vs effective oxygen yields, and the stellar, gas and baryonicmass vs SFE show higher dispersions and lower correlations. Since we use thedust mass as a tracer of gas mass, we derive the Dust-to-Gas Ratio and the COluminosity-to-molecular gas mass conversion factors, showing differences of0.16 and 0.95 dex for the total and molecular gas surface density,respectively, in comparison to previously reported values. We use a selfregulated feedback model to conclude that stellar feedback plays an importantrole generating outflows in NGC 1569.

Metal-THINGS: a panchromatic analysis of the local scaling relationships of the dwarf irregular galaxy NGC 1569