Free Access
Volume 580, August 2015
Article Number A125
Number of page(s) 16
Section Planets and planetary systems
Published online 17 August 2015

Online material

thumbnail Fig. 9

Correlations between the parameters derived from ESBL’s model discussed in Sect. 3.1. The red point refers to the best-fitting model obtained.

Open with DEXTER

thumbnail Fig. 10

Idem for ESBL+P’s model.

Open with DEXTER

thumbnail Fig. 11

Idem for ESBL+LOM’s model.

Open with DEXTER

thumbnail Fig. 12

Idem for ESBL+P+LOM’s model (u0> 0) with ρ′ = 5.3 × 10-4.

Open with DEXTER

© ESO, 2015

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