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Table 1:

Stellar properties of 30 Ari A, B.
Parameter 30 Ari A 30 Ari B
RA 02 37 00.5237 02 36 57.7405
Dec +24 38 50.0000 +24 38 53.0270
Spectral type F5V14 F4V4, F6V6, F6V14
$v\sin i$ [ $\rm km~s^{-1}$] $38.5\pm2.6^{14}$ 40.67, $38.3\pm1.8^{14}$
V [mag] 6.49710, 6.485 7.09110, 7.15
B-V [mag] 0.4108,13 0.51012,13
J [mag] $5.681\pm0.019^{11}$ $6.080\pm0.020^{11}$
H [mag] $5.580\pm0.051^{11}$ $5.908\pm0.029^{11}$
K [mag] $5.479\pm0.024^{11}$ $5.822\pm0.021^{11}$
Mv 3.4810, 3.465 4.1210, 4.125
$\pi$ [mas] $24.92\pm1.05^{3}$ $25.36\pm1.10^{3}$
Distance [pc] $40.1\pm1.7$ $39.4\pm1.7$
$\rm [Fe/H]$ [dex] 0.274, 0.0010, 0.271,7, -0.1310,
  0.112 $0.245\pm0.195^{9}$,
    0.032, 0.276
$T_{\rm eff}$ [K] 64624, 666810 64621,4, 615210
  $6300\pm60^{9}$, 67262 $6300\pm60^{9}$, 63642,
  64575 66075
$\log g$ 4.512, 4.255 4.504, 4.542, 4.445
$M_*~[M_\odot]$ $1.32\pm0.05^{10}$, 1.365 $1.11\pm0.06^{10}$, 1.205
  $1.31\pm0.04^{14}$ $1.16\pm0.04^{14}$
Age [Gyr] $0.86\pm0.63^{14}$ $0.91\pm0.83^{14}$
$R_*~[R_\odot]$ $1.37\pm0.03^{10}$ $1.13\pm0.03^{14}$
$\rm\theta~[mas]$ $0.32\pm0.01^{14}$ $0.26\pm0.01^{14}$

1 Boesgaard & Friel (1990). 2 Marsakov et al. (1995). 3 Hipparcos, Perryman & ESA (1997). 4 Cayrel de Strobel et al. (1997). 5 Allende Prieto et al. (1999). 6 Malagnini et al. (2000). 7 Buzzoni et al. (2001). 8 De Medeiros et al. (2002). 9 Taylor (2003). 10 Nordström et al. (2004). 11 Skrutskie et al. (2006). 12 Tolbert (1964). 13 Mermilliod (1991). 14 This work.


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