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Home All issues Volume 690 (October 2024) A&A, 690 (2024) A125 Full HTML
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Table A.3

Stellar parameters of the Miras inferred from the simulations.

Name P1.0 ∆P1.0 P1.5 ∆P1.5 log(𝑔1.0) log(𝑔1.5) R1.0 R1.5 T1.0 T1.5
[days] [%] [days] [%] [cgs] [cgs] [R⊙] [R⊙] [K] [K]
Y And 270 22 254 15 −0.35 −0.27 246 274 3012 3042
RT Aql 380 16 367 12 −0.52 −0.47 302 348 2843 2860
SY Aql 353 1 339 5 −0.48 −0.43 289 330 2879 2898
V335 Aql 225 28 209 19 −0.25 −0.16 221 242 3106 3144
T Aqr 213 5 197 2 −0.22 −0.13 214 232 3136 3177
U Ari 402 8 390 5 −0.55 −0.50 312 362 2816 2830
RU Aur 443 6 434 8 −0.60 −0.56 331 387 2770 2780
R Boo 261 17 245 10 −0.33 −0.25 241 268 3029 3061
T Cap 337 25 323 19 −0.46 −0.40 281 320 2901 2922
CM Car 246 28 230 32 −0.30 −0.21 233 257 3060 3095
U Cet 298 27 283 21 −0.40 −0.33 261 293 2962 2989
R Cha 270 20 254 25 −0.35 −0.27 246 274 3012 3042
S CMi 371 11 358 7 −0.51 −0.46 298 342 2854 2872
U CMi 283 31 267 35 −0.37 −0.29 253 283 2988 3017
W Cnc 464 18 456 16 −0.63 −0.59 340 400 2748 2757
R Col 231 30 215 35 −0.27 −0.17 224 246 3093 3130
T Col 207 9 191 16 −0.21 −0.11 210 228 3151 3194
RY CrA 262 27 247 20 −0.33 −0.25 242 269 3026 3058
X CrB 215 11 199 17 −0.23 −0.13 215 234 3130 3171
R Del 277 3 261 9 −0.36 −0.28 250 279 2999 3028
W Dra 184 36 169 42 −0.15 −0.04 196 210 3212 3260
T Eri 281 11 265 5 −0.37 −0.29 252 282 2992 3021
U Eri 239 13 223 19 −0.28 −0.19 229 252 3075 3111
V Gem 402 46 391 42 −0.55 −0.5 312 362 2815 2829
S Her 261 14 245 19 −0.33 −0.25 242 268 3028 3061
SV Her 215 10 199 16 −0.23 −0.13 215 234 3130 3170
T Her 206 26 190 16 −0.21 −0.11 210 227 3153 3195
T Hor 227 4 211 4 −0.26 −0.16 222 243 3102 3140
RR Hya 290 15 274 20 −0.38 −0.31 257 288 2976 3004
RU Hya 332 1 317 5 −0.45 −0.39 279 316 2908 2930
S Lac 242 1 226 6 −0.29 −0.20 231 254 3067 3103
RR Lib 302 9 287 3 −0.4 −0.33 263 296 2956 2982
R LMi 482 29 475 27 −0.65 −0.61 348 411 2730 2737
RT Lyn 258 34 243 38 −0.32 −0.24 240 266 3034 3067
U Oct 240 21 224 26 −0.29 −0.20 230 253 3072 3108
R Oph 393 30 381 26 −0.54 −0.49 308 356 2827 2842
RY Oph 252 67 236 57 −0.31 −0.23 236 261 3047 3081
SY Pav 219 15 203 6 −0.24 −0.14 217 237 3121 3161
R Peg 421 11 410 9 −0.58 −0.53 321 373 2794 2806
S Peg 331 5 316 1 −0.45 −0.39 278 316 2910 2932
X Peg 209 4 194 4 −0.22 −0.12 212 230 3144 3186
Z Peg 264 19 248 24 −0.33 −0.25 243 270 3023 3055
RZ Sco 274 72 258 62 −0.35 −0.28 249 277 3004 3034
R Sgr 326 21 311 16 −0.44 −0.38 275 312 2918 2941
RV Sgr 286 10 270 15 −0.38 −0.30 255 285 2983 3012
BH Tel 264 22 248 14 −0.33 −0.25 243 270 3024 3056
T Tuc 219 11 203 18 −0.24 −0.14 218 237 3120 3159
T UMa 279 9 263 3 −0.36 −0.29 251 280 2996 3025
RR UMa 209 10 193 16 −0.21 −0.12 212 230 3145 3186
T UMi 236 1 220 6 −0.28 −0.19 227 250 3081 3118
CI Vel 173 25 158 14 −0.12 0.00 189 201 3247 3297
R Vir 236 62 220 51 −0.28 −0.19 227 250 3081 3118
R Vul 226 66 211 54 −0.26 −0.16 222 243 3103 3141

Notes. The subscripts 1.0 denotes quantities derived from the 1.0 M⊙ simulations, and 1.5 those from the 1.5 M⊙ simulations. The columns are: Miras’ name; the pulsation periods P1.0 and P1.5 in days; the relative difference between the observed pulsation period and our results ∆P1.0 and ∆P1.5 in %; the effective surface gravity log(g1.0) and log(g1.5), with 𝑔 in cgs; R1.0 and R1.5 the radius in R⊙; T1.0 and T1.5 the effective temperature in K.

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