. . . . . . . . . . "aa16643-11" . . "2012"^^ . . "\u00A9 ESO, 2012" . . "Tidal dissipation in multi-planet systems and constraints on orbit fitting"@en . "ESO" . . . "2012"^^ . . "We present here in full detail the linear secular theory with tidal damping that was used to constrain the fit to the HD\u00A010180 planetary system in Lovis et al. (2011, A&A, 528, A112). The theory is very general and can provide some intuitive understanding of the final state of a planetary system when one or more planets are close to their central star. We globally recover the results of Mardling (2007, MNRAS, 382, 1768). However, for the HD\u00A0209458 planetary system, we show that the consideration of the tides raised by the central star on the planet leads one to believe that the eccentricity of HD\u00A0209458b is most probably much smaller than 0.01."@en . .