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Home All issues Volume 495 / No 3 (March I 2009) A&A, 495 3 (2009) 901-917 Full HTML
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Table 3:

Stellar fluxes, masses, luminosities, ages and distances.

Star		 F* (W m-2) $M_*/M_\odot$ $L_*/L_\odot$ Age (Myr) d (pc) $d_{\rm Hip}$ (pc) $d_{\rm other}$ (pc)
HD 31648 $3.308\times 10^{-11}$ $\rm 1.97^{+0.04}_{+0.45}$ $\rm 21.9^{-7.8}_{+20.7}$ $\rm 6.7^{+1.0}_{-3.3}$ $\rm 146^{-29}_{+57}$ $\rm 137^{+31}_{-21}$  
HD 58647 $9.940\times 10^{-11}$ $\rm 5.99^{-0.36}_{+0.38}$ $\rm 911.2^{-113.4}_{+221.2}$ $\rm0.4^{+0.1}_{-0.1}$ $\rm 543^{-35}_{+62}$    
HD 150193 $2.825\times 10^{-11}$ $\rm 2.22^{-0.04}_{+0.27}$ $\rm 36.1^{-9.2}_{+17.5}$ $\rm 5.0^{+0.5}_{-1.5}$ $\rm 203^{-28}_{+44}$    
HD 163296 $6.583\times 10^{-11}$ $\rm 2.25^{+0.11}_{+0.07}$ $\rm 34.5^{-5.1}_{+9.3}$ $\rm 5.0^{-0.3}_{-0.6}$ $\rm 130^{-10}_{+16}$ $\rm 119^{+12}_{-10}$  
HD 179218 $4.996\times 10^{-11}$ $\rm 2.56^{-0.16}_{+0.21}$ $\rm 63.1^{-12.8}_{+17.0}$ $\rm 3.3^{+0.7}_{-0.7}$ $\rm 201^{-22}_{+25}$    
HD 190073 $2.575\times 10^{-11}$ $\rm 5.05^{-0.47}_{+0.54}$ $\rm 470.8^{-88.2}_{-189.2}$ $\rm0.6^{+0.2}_{-0.2}$ $\rm 767^{-76}_{+139}$    
HR 10 $1.737\times 10^{-10}$ $\rm 3.30^{-0.37}_{+0.43}$ $\rm 140.3^{-41.9}_{+59.2}$ $\rm 1.8^{+0.5}_{-0.5}$ $\rm 161^{-26}_{+31}$ $\rm 176^{+24}_{-19}$  
HR 2174 $1.515\times 10^{-10}$ $\rm 6.82^{-0.93}_{+1.02}$ $\rm 1012.7^{-351.4}_{+217.2}$ $\rm0.2^{+0.1}_{-0.1}$ $\rm 463^{-89}_{+47}$    
HR 9043 $8.784\times 10^{-11}$ $\rm 2.07^{-0.21}_{+0.27}$ $\rm 23.7^{-6.7}_{+10.0}$ $\rm 5.5^{+2.0}_{-1.7}$ $\rm 93^{-14}_{+18}$ $\rm 88^{+4}_{-3}$  
AS 442 $9.753\times 10^{-12}$ $\rm 3.54^{-0.37}_{+0.44}$ $\rm 207.2^{-60.1}_{+85.2}$ $\rm 1.5^{+0.5}_{-0.5}$ $\rm 826^{-130}_{+155}$    
BD+31 643 $2.483\times 10^{-10}$ $\rm 6.15^{-0.29}_{+0.29}$ $\rm 1663.5^{-234.9}_{+329.8}$ $\rm0.4^{+0.1}_{-0.1}$ $\rm 464^{-34}_{+36}$    
$\lambda $ Boo $6.240\times 10^{-10}$ $\rm 1.66^{-0.16}_{+0.19}$ $\rm 19.1^{-6.1}_{+9.0}$ $\rm 2.8^{+1.1}_{-0.8}$ $\rm 31^{-5}_{+7}$ $30\pm 1$  
VX Cas $2.589\times 10^{-12}$ $\rm 2.33^{-0.03}_{+0.14}$ $\rm 30.8^{-5.7}_{+5.8}$ $\rm 6.4^{+4.0}_{-1.5}$ $\rm 619^{-60}_{+58}$   $\rm 760^{1,3}$
SV Cep $3.390\times 10^{-12}$ $\rm 2.45^{-0.08}_{+0.26}$ $\rm 37.5^{-5.1}_{+14.5}$ $\rm 5.2^{+1.4}_{-2.1}$ $\rm 596^{-43}_{+106}$   4403
24 CVn $4.686\times 10^{-10}$ $\rm 2.64^{-0.11}_{+0.42}$ $\rm 65.9^{-19.1}_{+38.0}$ $\rm 3.1^{+0.6}_{-1.1}$ $\rm 67^{-11}_{+17}$ $55\pm 1$  
51 Oph $4.991\times 10^{-10}$ $\rm 4.22^{-0.30}_{+0.33}$ $\rm 312.3^{-62.3}_{+72.0}$ $\rm0.7^{+0.4}_{-0.5}$ $\rm 142^{-15}_{+15}$ $124\pm 4$  
T Ori $7.242\times 10^{-12}$ $\rm 2.42^{+0.06}_{+0.17}$ $\rm 50.2^{-9.4}_{+17.4}$ $\rm 4.0^{-0.1}_{-0.8}$ $\rm 472^{-46}_{+76}$   4601
BF Ori $5.445\times 10^{-12}$ $\rm 2.61^{-0.25}_{+0.41}$ $\rm 61.6^{-20.2}_{+32.4}$ $\rm 3.2^{+1.3}_{-0.9}$ $\rm 603^{-109}_{+142}$   4502, 4303
UX Ori $4.414\times 10^{-12}$ $\rm 2.26^{-0.25}_{+0.52}$ $\rm 36.8^{-13.7}_{+30.5}$ $\rm 4.5^{+2.0}_{-2.3}$ $\rm 517^{-108}_{+182}$   4601, 4002, 3403
V346 Ori $5.752\times 10^{-12}$ $\rm 2.52^{-0.11}_{+0.31}$ $\rm 61.4^{-15.8}_{+27.3}$ $\rm 3.5^{+0.6}_{-1.1}$ $\rm 586^{-81}_{+118}$   4502
V350 Ori $1.741\times 10^{-12}$ $\rm 2.16^{+0.13}_{+0.13}$ $\rm 29.29^{-5.8}_{+11.6}$ $\rm 5.5^{-0.1}_{-1.0}$ $\rm 735^{-77}_{+133}$   4601, 4502
XY Per $2.290\times 10^{-11}$ $\rm 2.79^{-0.36}_{+0.59}$ $\rm 85.6^{-34.0}_{+64.3}$ $\rm 2.5^{+1.5}_{-0.8}$ $\rm 347^{-78}_{+190}$   1201, 3502, 1603
VV Ser 2.869 $\times 10^{-11}$ $\rm 3.95^{+0.15}_{+0.41}$ $\rm 336.2^{-89.4}_{+117.2}$ $\rm 1.2^{+0.1}_{-0.5}$ $\rm 614^{-88}_{+99}$   4401, 3303, 2304
17 Sex $1.757\times 10^{-10}$ $\rm 6.35^{-0.74}_{+0.80}$ $\rm 940.5^{-277.2}_{+295.8}$ $\rm0.3^{+0.1}_{-0.1}$ $\rm 415^{-30}_{+61}$    
RR Tau $5.673\times 10^{-12}$ $\rm 5.79^{-0.94}_{+0.99}$ $\rm 780.5^{-351.9}_{+446.7}$ $\rm0.4^{+0.3}_{-0.2}$ $\rm 2103^{-544}_{+535}$   8001, 6002
WW Vul $3.315\times 10^{-12}$ $\rm 2.50^{-0.06}_{+0.48}$ $\rm 50.0^{-19.11}_{+44.5}$ $\rm 3.7^{+3.7}_{-1.7}$ $\rm 696^{-149}_{+261}$   5501, 5342

HR 26 A		 $2.582\times 10^{-10}$ $\rm 3.08^{-0.07}_{+0.07}$ $\rm 106.9^{-14.2}_{+15.7}$ $\rm 175^{-23}_{+14}$ $\rm 115^{-8}_{+8}$ $94\pm3$  
    $\rm 3.01^{+0.10}_{-0.01}$ $\rm 104.0^{-7.8}_{+11.9}$ $\rm 2.6^{-0.2}_{-0.1}$ $\rm 114^{-4}_{+6}$    
HR 4757 A $2.647 \times 10^{-9}$ $\rm 2.74^{-0.06}_{+0.07}$ $\rm 69.0^{-8.9}_{+9.7}$ $\rm 260^{-24}_{+14}$ $\rm 29^{-2}_{+2}$ $27 \pm 1$  
    $\rm 2.64^{+0.04}_{+0.02}$ $\rm 64.0^{-4.2}_{+10.7}$ $\rm 3.2^{-0.1}_{-0.1}$ $\rm 28^{-1}_{+2}$    
HR 5422 A $1.439\times 10^{-10}$ $\rm 2.66^{-0.07}_{+0.08}$ $\rm 60.4^{-9.8}_{+11.0}$ $\rm 267^{-39}_{+23}$ $\rm 116^{-10}_{+10}$ $110 \pm 5$  
    $\rm 2.59^{+0.09}_{+0.01}$ $\rm 58.5^{-5.7}_{+8.7}$ $\rm 3.4^{-0.2}_{-0.1}$ $\rm 114^{-6}_{+8}$    
49 Cet $2.064\times 10^{-10}$ $\rm 2.17^{-0.03}_{+0.06}$ $\rm 21.8^{-1.0}_{+3.9}$ $\rm 61^{-46}_{+119}$ $\rm 58^{-1}_{+5}$ $59 \pm 1$  
    $\rm 2.15^{-0.01}_{+0.11}$ $\rm 21.6^{-0.8}_{+4.4}$ $\rm 8.9^{+6.1}_{-2.4}$ $\rm 58^{-1}_{+6}$    
Notes to Table 3: A discussion on the derivation of the distances in Col. 6 is given in Sect. 6.3. The distances given in Col. 8 are taken from the works by 1 Hernández et al. (2004), 2 Blondel & Tjin A Djie (2006), 3 Manoj et al. (2006) and 4 Eiroa et al. (2008); see those works for the original references. For HR 26 A, HR 4757 A, HR 5422 A and 49 Cet we give the solutions derived using both Post-MS and PMS tracks, respectively (see Sect. 6.4).

Source LaTeX | All tables | In the text

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