Table A.1
RHD simulation parameters.
Id | Simulation | M★ | L★ | R★ | Teff | log 𝑔 | tavg | Ppuls | σPpuls | 〈Px〉 | 〈Py〉 | σP | σP |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
[M⊙] | [L⊙] | [R⊙] | [K] | [cgs] | [yr] | [days] | [days] | [AU] | [AU] | [AU] | % [R★] | ||
1 | st28gm05n038 | 1.0 | 4978 | 281 | 2893 | −0.46 | 19.05 | 341 | 31 | −0.025 | −0.004 | 0.108 | 8.26 |
2 | st28gm05n043 | 1.0 | 5013 | 278 | 2908 | −0.45 | 19.03 | 337 | 30 | −0.011 | −0.044 | 0.113 | 8.74 |
3 | st28gm06n057 | 1.0 | 7055 | 349 | 2831 | −0.65 | 15.87 | 485 | 77 | 0.012 | 0.005 | 0.152 | 9.37 |
4 | st28gm06n059 | 1.0 | 7050 | 347 | 2837 | −0.64 | 15.87 | 487 | 77 | 0.082 | −0.055 | 0.143 | 8.86 |
5 | st28gm07n006 | 1.0 | 8003 | 379 | 2801 | −0.72 | 15.85 | 546 | 99 | −0.055 | 0.011 | 0.219 | 12.43 |
6 | st28gm07n008 | 1.0 | 8020 | 377 | 2812 | −0.72 | 15.84 | 541 | 102 | 0.006 | −0.029 | 0.171 | 9.75 |
7 | st28gm08n001 | 1.0 | 8980 | 408 | 2780 | −0.78 | 19.39 | 592 | 129 | −0.141 | −0.018 | 0.202 | 10.65 |
8 | st29gm02n013 | 1.0 | 2983 | 190 | 3092 | −0.12 | 11.23 | 178 | 13 | −0.015 | −0.012 | 0.052 | 5.89 |
9 | st29gm03n001 | 1.0 | 3990 | 241 | 2955 | −0.33 | 15.22 | 262 | 18 | 0.001 | −0.001 | 0.094 | 8.39 |
10 | st29gm03n002 | 1.0 | 4028 | 241 | 2964 | −0.33 | 15.22 | 263 | 18 | 0.008 | −0.008 | 0.133 | 11.87 |
11 | st31gm01n002 | 1.0 | 2500 | 165 | 3177 | 0.01 | 9.13 | 134 | 14 | −0.002 | −0.003 | 0.028 | 3.65 |
12 | st32g01n002 | 1.0 | 1978 | 138 | 3275 | 0.16 | 7.02 | 98 | 8 | −0.006 | −0.007 | 0.025 | 3.90 |
13 | st28gm05n006 | 1.5 | 4985 | 269 | 2957 | −0.25 | 15.85 | 240 | 20 | −0.003 | 0.004 | 0.087 | 6.95 |
14 | st28gm05n008 | 1.0 | 4942 | 302 | 2786 | −0.52 | 15.85 | 387 | 36 | 0.003 | −0.032 | 0.067 | 4.77 |
15 | st28gm05n017 | 1.5 | 7490 | 321 | 2994 | −0.40 | 15.86 | 328 | 22 | −0.013 | −0.072 | 0.129 | 8.64 |
16 | st28gm05n020 | 1.5 | 7708 | 327 | 2989 | −0.42 | 15.86 | 351 | 30 | −0.046 | −0.023 | 0.130 | 8.55 |
17 | st28gm05n022 | 1.0 | 5068 | 312 | 2757 | −0.55 | 15.85 | 422 | 42 | 0.005 | −0.027 | 0.086 | 5.93 |
18 | st28gm05n028 | 1.5 | 6946 | 306 | 3009 | −0.36 | 15.85 | 298 | 16 | 0.028 | −0.015 | 0.104 | 7.31 |
19 | st28gm05n029 | 1.5 | 6941 | 288 | 3102 | −0.31 | 15.70 | 278 | 15 | 0.024 | −0.010 | 0.093 | 6.94 |
20 | st28gm05n034 | 1.5 | 6880 | 278 | 3150 | −0.28 | 7.93 | 259 | 14 | −0.004 | −0.040 | 0.082 | 6.34 |
21 | st28gm06n032 | 1.0 | 7062 | 339 | 2872 | −0.62 | 15.87 | 508 | 69 | −0.034 | 0.011 | 0.156 | 9.90 |
22 | st28gm06n043 | 1.0 | 7079 | 344 | 2854 | −0.64 | 15.87 | 461 | 75 | −0.062 | −0.041 | 0.108 | 6.75 |
23 | st28gm06n053 | 1.5 | 10073 | 391 | 2922 | −0.57 | 15.85 | 418 | 46 | 0.009 | −0.068 | 0.238 | 13.09 |
24 | st26gm07n002 | 1.0 | 6986 | 439 | 2524 | −0.85 | 25.35 | 594 | 112 | −0.100(a) | 0.046(a) | 0.187(a) | 9.16(a) |
25 | st26gm07n001 | 1.0 | 6953 | 402 | 2635 | −0.77 | 27.74 | 517 | 94 | −0.098(a) | 0.024(a) | 0.198(a) | 10.59(a) |
26 | st28gm06n026 | 1.0 | 6955 | 372 | 2737 | −0.70 | 25.35 | 471 | 116 | −0.068(a) | −0.002(a) | 0.152(a) | 8.79(a) |
27 | st29gm06n001 | 1.0 | 6995 | 324 | 2929 | −0.59 | 31.70 | 389 | 73 | −0.098(a) | 0.016(a) | 0.174(a) | 11.55(a) |
28 | st27gm06n001 | 1.0 | 5011 | 322 | 2704 | −0.58 | 31.73 | 450 | 38 | −0.027 | 0.027 | 0.090 | 6.01 |
29 | st28gm05n002 | 1.0 | 4978 | 314 | 2742 | −0.56 | 25.35 | 393 | 38 | −0.002(a) | 0.033(a) | 0.077(a) | 5.27(a) |
30 | st28gm05n001 | 1.0 | 5019 | 289 | 2858 | −0.49 | 31.83 | 360 | 44 | −0.057 | 0.017 | 0.097 | 7.22 |
31 | st29gm04n001 | 1.0 | 4982 | 295 | 2827 | −0.50 | 25.35 | 339 | 37 | −0.002(a) | 0.023(a) | 0.078(a) | 5.69(a) |
Notes. The simulations 1-12 are the new models presented in this work; the simulations 13-23 are presented in Ahmad et al. (2023) and the simulations 24-31 are presented in Freytag et al. (2017) and Chiavassa et al. (2018). The table displays the simulation name, the stellar mass M★, the average emitted luminosity L★, the average approximate stellar radius R★, the effective temperature Teff, the surface gravity log(g), the pulsation period Ppuls, the spread in the pulsation period i.e. the pulsation period uncertainty σpuls, and the stellar time tavg used for the averaging of the rest of the quantities. The stellar parameters may slightly vary from original articles as they are updated thanks to Ahmad’s and Freytag’s work. The last four columns are the time-averaged positions Px and Py in AU and the standard deviation of the photocentre displacement σP (in AU and in % of R★). Data denoted by the footnote (a) come from the previous analysis of Chiavassa et al. (2018).
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