Fig. 13
Time evolution of eccentricity of planets embedded in isothermal discs with H/r = 0.037 and individual starting eccentricity. The vertical dotted line at t = 10 indicates the time at which the planets have grown to their full mass. The black dashed lines indicate an exponential decay with a fitted τecc = 29 shifted to obtain a match for e0 = 0.1,0.2,0.3 and 0.4.
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