File:Red giant simulation 3.jpg

English: Probing red supergiant dynamics through photo-center displacements measured by Gaia paper. Example of intensity maps in Gaia G photometric system for two RHD simulations in Table 1 and for two different snapshots about 200 days apart. The range is [0.−825942] erg s−1 cm−2 Å−1 for low Teff and log g simulation st35gm04n38 (top panel) and [0.−299977] erg s−1 cm−2 Å−1 for the highest Teff and log g simulation st36gm00n05 (bottom panel). The intensity is shown on a square-root scale to make the structures more visible.