Continuum and spectral line results towards the ALMAGAL field 865468 (also labelled AG345.0035–0.2240 in Molinari et al. 2025). From top to bottom, results for the 7M (beam size of $7_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}3\times 4_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}7$), 7M+TM2 (beam size of $2_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}1\times 1_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}7$), and 7M+TM2+TM1 (beam size of $0_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}36\times 0_{\cdot }^{\mathrm{\prime }\mathrm{\prime }}34$) images. The left-column panels show the dust continuum emission at 219 GHz (or 1.38 mm). The middle-column panels show the spectra towards different compact sources identified in the continuum images. The right-column panels show the emission for two molecular spectral lines: SiO (5–4) and CH₃CN (12_K=3−11_K=3). The color image shows the first order moment map, or velocity field of the CH₃CN line over a velocity range from −37 to −17 km s⁻¹ (the systemic velocity of the region is −27 km s⁻¹). The blue and red contours show zero-th order moment maps (or integrated emission) of the blue-shifted (from −100 to −37 km s⁻¹) and red-shifted (from −17 to 46 km s⁻¹) SiO emission, respectively. The black contour depicts the spatial distribution of the continuum emission as shown in the left-column panels.