Worldwide astronomical and astrophysical research
| Issue |
A&A
Volume 580, August 2015
|
|
|---|---|---|
| Article Number | A125 | |
| Number of page(s) | 16 | |
| Section | Planets and planetary systems | |
| DOI | https://doi.org/10.1051/0004-6361/201525791 | |
| Published online | 17 August 2015 | |
 |
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 | |
 |
Fig. 10
Idem for ESBL+P’s model. |
| Open with DEXTER | |
 |
Fig. 11
Idem for ESBL+LOM’s model. |
| Open with DEXTER | |
 |
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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