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Home All issues Volume 501 / No 2 (July II 2009) A&A, 501 2 (2009) 769-776 Full HTML
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Table 3:

Best-fit solutions of the two methods the system of 809 Lundia based on the fit of photometric observations made in 2005-2006 and 2006-2007 (see Fig. 9).
Model Component A Component B Separation Mass Density Period Pole of orbit
  km km km ratio $\rm g/cm^3$ h $\lambda$ deg $\beta$ deg
  a b c a' b' c'            
Modified 3.9 3.3 3.2 3.5 2.9 2.8 15.8 0.7 $\pm $ 0.1 1.64 $\pm $ 0.1 15.418 $\pm $ 0.001 119 $\pm $ 2 28 $\pm $ 4
Roche                        
Kinematic 4.1 3.3 2.5 3.2 2.9 2.7 15.8 0.7 $\pm $ 0.1 1.71 $\pm $ 0.1 15.418 $\pm $ 0.001 120 $\pm $ 5 18 $\pm $ 12

Source LaTeX | All tables | In the text

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