Figure 1.
Intensity (top panels) and velocity (bottom panels) maps of the stars, H i, molecular gas, and ionized gas in the Fornax dwarfs. Top-left panels: white-light image/stellar kinematics, respectively, top-right panels: H i maps, bottom-left panels, ionized gas maps, and bottom-right panels: molecular gas maps. The 11 arcsec H i maps are shown, with the outermost contour of the 22 arcsec map shown in light red. The corresponding beams of the H i and CO observations are shown in the respective bottom-left corners, and a scale bar is shown in the bottom-left corner of the ionized gas maps. The arrow in the top-right corner of the H i intensity panel indicates the projected direction to the cluster centre. Contours of the MUSE white-light (in log-scale) image are overlaid on each panel for scale. Additionally, the sizes of the bottom panels are indicated in the top-left panels with dashed rectangles.

Intensity (top panels) and velocity (bottom panels) maps of the stars, H i, molecular gas, and ionized gas in the Fornax dwarfs. Top-left panels: white-light image/stellar kinematics, respectively, top-right panels: H i maps, bottom-left panels, ionized gas maps, and bottom-right panels: molecular gas maps. The 11 arcsec H i maps are shown, with the outermost contour of the 22 arcsec map shown in light red. The corresponding beams of the H i and CO observations are shown in the respective bottom-left corners, and a scale bar is shown in the bottom-left corner of the ionized gas maps. The arrow in the top-right corner of the H i intensity panel indicates the projected direction to the cluster centre. Contours of the MUSE white-light (in log-scale) image are overlaid on each panel for scale. Additionally, the sizes of the bottom panels are indicated in the top-left panels with dashed rectangles.

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