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Table 1

Basic model parameters and derived quantities.

Model M Menv L nx3$\[n_{x}^{3}\]$ xbox tavg R⋆,smin Teff,smin log gsmin Ppuls
(M) (M) (L) (R) (yr) (R) (K) cgs (d)
st28gm06n051 1.0 0.182 6933 6373 1558 48.27 328 2907 −0.598 459
st28gm05n056 1.0 0.399 5085 3173 1263 60.20 293 2848 −0.498 390 Shock, Sect. 5
st28gm05n032 1.5 0.256 6936 6373 1263 24.93 280 3149 −0.286 256
st35gm04n048 5.0 0.110 40914 6373 1929 26.58 623 3288 −0.456 523 Rebound, Sect. 4
st35gm04n045 5.0 0.092 41336 6373 1929 20.91 597 3368 −0.419 516 Plume, Sect. 3
st34gm02n002 8.0 0.277 41675 7653 1626 23.17 602 3359 −0.223 314

Notes. The table shows the model name (composed of “s,” referring to the gravitational potential, “t” for “temperature” followed by two digits indicating the approximate effective temperature, “g” for “gravity” followed by “m” for “minus” and two digits indicating the approximate logarithm of the surface gravity, and “n” for “number” with the model counter); the current stellar mass, M, used for prescribing the gravitational potential; the envelope mass, Menv, derived from integrating the mass density of all grid cells within the computational box; the average emitted luminosity, L; the grid dimensions, nx3$\[n_{x}^{3}\]$; the edge length of the cubical computational box, xbox; the time, tavg, used for averaging the remaining quantities in this table; the average approximate stellar radius, R⋆,smin, taken as the radial position of the innermost photospheric entropy minimum (see Ahmad et al. 2023); the average approximate effective temperature, Teff,smin; the logarithm of the average approximate surface gravity, log gsmin; the pulsation period, Ppuls; and a comment about the levitation mechanism that we used the model as a reference for. The first three models (with M = 1 and 1.5 M) are examples of the scenario of darkening due to cool post-shock gas (see Sect. 5). The 5 M model st35gm04n048 shows a prominent dimming event due to a convective rebound (we present in Sect. 4). The remaining two models (with M = 5 and 8 M) show dark patches due to plumes (see Sect. 3).

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