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Table 3.

Derived parameters of 30 galactic RRd stars.

Target log LG log Teff log M log L [M/H] Age DML
V0500 Hya 1.764 ± 0.027 3.8175 −0.127 ± 0.008 1.742 ± 0.028 −1.88 ± 0.50 61 ± 16 0.0003
V0372 Ser 1.639 ± 0.022 3.8189 −0.160 ± 0.012 1.622 ± 0.011 −1.18 ± 0.05 25 ± 14 0.0379
Z Gru 1.604 ± 0.030 3.8289 −0.170 ± 0.008 1.677 ± 0.015 −1.40 ± 0.06 56 ± 24 0.0002
XX Crv 1.751 ± 0.031 3.8271 −0.131 ± 0.001 1.762 ± 0.023 −2.18 ± 0.50 68 ± 02 0.0001
V0381 Tel 1.657 ± 0.042 3.8304 −0.181 ± 0.003 1.649 ± 0.019 −1.18 ± 0.11 40 ± 15 0.0003
AQ Leo 1.783 ± 0.037 3.8192 −0.117 ± 0.010 1.743 ± 0.030 −1.88 ± 0.35 56 ± 28 0.0002
V5644 Sgr 1.826 ± 0.054 3.8283 −0.191 ± 0.004 1.623 ± 0.025 −1.04 ± 0.12 48 ± 00 0.0060
NN Boo 1.655 ± 0.031 3.8268 −0.176 ± 0.001 1.646 ± 0.021 −1.18 ± 0.11 30 ± 14 0.0069
BS Com 1.693 ± 0.042 3.8327 −0.148 ± 0.013 1.711 ± 0.032 −1.70 ± 0.30 59 ± 06 0.0002
V0363 Dra 1.701 ± 0.033 3.8220 −0.127 ± 0.011 1.739 ± 0.031 −1.88 ± 0.32 60 ± 08 0.0002
SW Ret 1.487 ± 0.043 3.8217 −0.166 ± 0.007 1.635 ± 0.015 −1.18 ± 0.05 27 ± 00 0.0237
AL Vol 1.690 ± 0.027 3.8274 −0.129 ± 0.020 1.735 ± 0.005 −1.88 ± 0.00 59 ± 25 0.0003
V0374 Tel 1.795 ± 0.066 3.8243 −0.172 ± 0.003 1.643 ± 0.019 −1.18 ± 0.11 28 ± 08 0.0122
AZ For 1.725 ± 0.036 3.8182 −0.125 ± 0.008 1.772 ± 0.015 −2.40 ± 0.26 68 ± 05 0.0002
CZ Phe 1.720 ± 0.037 3.8196 −0.104 ± 0.021 1.772 ± 0.005 −2.18 ± 0.15 62 ± 11 0.0002
V0338 Boo 1.669 ± 0.040 3.8207 −0.174 ± 0.005 1.643 ± 0.018 −1.18 ± 0.07 26 ± 17 0.0119
V0458 Her 1.880 ± 0.045 3.8253 −0.169 ± 0.002 1.657 ± 0.020 −1.28 ± 0.11 21 ± 16 0.0078
XY Crv 1.803 ± 0.044 3.8309 −0.174 ± 0.001 1.678 ± 0.021 −1.40 ± 0.13 60 ± 23 0.0002
V0416 Pav 1.586 ± 0.031 3.8204 −0.164 ± 0.006 1.647 ± 0.016 −1.18 ± 0.05 26 ± 01 0.0175
CU Com 1.794 ± 0.057 3.8207 −0.121 ± 0.011 1.741 ± 0.013 −1.88 ± 0.09 58 ± 29 0.0003
CR Cap 1.636 ± 0.067 3.8281 −0.164 ± 0.009 1.661 ± 0.029 −1.40 ± 0.18 02 ± 11 0.0068
AG PsA 1.635 ± 0.045 3.8305 −0.119 ± 0.001 1.735 ± 0.021 −1.88 ± 0.15 54 ± 09 0.0004
V2493 Oph 1.657 ± 0.042 3.8340 −0.168 ± 0.008 1.670 ± 0.015 −1.40 ± 0.05 28 ± 18 0.0003
BN UMa 1.711 ± 0.059 3.8166 −0.144 ± 0.007 1.697 ± 0.027 −1.54 ± 0.17 27 ± 13 0.0013
ASAS J211848-3430.4 1.729 ± 0.063 3.8150 −0.145 ± 0.008 1.657 ± 0.015 −1.40 ± 0.06 24 ± 02 0.0275
V0633 Cen 1.707 ± 0.062 3.8400 −0.182 ± 0.017 1.706 ± 0.008 −1.54 ± 0.00 72 ± 09 0.0002
QW Aqr 1.663 ± 0.075 3.8328 −0.174 ± 0.005 1.677 ± 0.017 −1.40 ± 0.07 60 ± 32 0.0002
ASAS J040054-4923.8 1.718 ± 0.050 3.8196 −0.134 ± 0.001 1.740 ± 0.021 −1.88 ± 0.24 64 ± 08 0.0003
ASAS J141539+0010.1 1.674 ± 0.072 3.8318 −0.155 ± 0.016 1.693 ± 0.035 −1.54 ± 0.30 54 ± 20 0.0002
CF Del 1.832 ± 0.105 3.8250 −0.172 ± 0.002 1.646 ± 0.020 −1.18 ± 0.11 29 ± 04 0.0103

Notes. Except for the Gaia luminosities (LG), all errors show the variations caused by a change of ±0.005 in log Teff as given in this table. Mass and luminosity are in solar units, the metal abundance [M/H] is given for Z = 0.0152, and the age is given in Myr and counted from the ZAHB. The last column shows the distance of the closest points between the pulsation and evolutionary models in the log L − log M plane (see Eq. (11)).

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