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Home All issues Volume 497 / No 2 (April II 2009) A&A, 497 2 (2009) 595-609 Full HTML
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Table 1:

Parameters of the model systems considered.
Planet m ( ${M}_{\rm J}$) a (AU) P (days) e $\zeta $
GJ 8761 c 0.790 0.131 30.46 0.263 $10\ensuremath{^\circ} $
b 2.530 0.208 60.83 0.031  
GJ 876 LM2 c 0.13 0.131 30.46 0.263 $10\ensuremath{^\circ} $
b 0.42 0.208 60.83 0.031  
GJ 876 SE3 c 0.013 0.131 30.46 0.263 $10\ensuremath{^\circ} $
b 0.042 0.208 60.83 0.031  
GJ 876 E4 c 0.0013 0.0131 30.46 0.263 $10\ensuremath{^\circ} $
b 0.0042 0.208 60.83 0.031  
GJ 876 LM HE5 c 0.13 0.131 30.46 0.41 $10\ensuremath{^\circ} $
b 0.42 0.208 60.83 0.09  
GJ 876 SE HE6 c 0.013 0.131 30.46 0.41 $10\ensuremath{^\circ} $
b 0.042 0.208 60.83 0.09  
HD 1283117 b 1.56 1.109 476.8 0.38 $58 \ensuremath{^\circ} $
c 3.08 1.735 933.1 0.21  
1 Orbital elements of the system (Obj)GJ 876(Obj) (Rivera et al. 2005, orbital inclination $i=50\ensuremath{^\circ} $).
2 Planet masses scaled down by a factor of 6. Equivalent to a Jovian mass planet around a solar mass star.
3 Planet masses scaled down by a factor of 60. Equivalent to a super-Earth around a solar mass star.
4 Planet masses scaled down by a factor of 600. Equivalent to an Earth mass planet around a solar mass star.
5 Planet masses scaled down by a factor of 6 (Jovian mass planet) and higher eccentricities than in the observed system.
6 Planet masses scaled down by a factor of 60 (super-Earth) and higher eccentricities than in the observed system.
7 Orbital elements of the system (Obj)HD 128311(Obj) (Vogt et al. 2005).

Source LaTeX | All tables | In the text

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