| Issue |
A&A
Volume 581, September 2015
|
|
|---|---|---|
| Article Number | A37 | |
| Number of page(s) | 12 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201526520 | |
| Published online | 31 August 2015 | |
Online material
Appendix A: Individual data sets and model curves
In this section we present the resulting phase diagrams for photometric and RV data sets for our studied stars. The diagrams are constructed by folding the data as Eq. (1) with the resulting orbital ephemerides (Table 2). Figures A.1−A.8 show individual data sets together with the phased model curves.
 |
Fig. A.1
Phase diagrams for A36 using the Pemp and Ṗemp from Table 2. Blue dashed lines in the magnitude plots denote a model light curve from PHOEBE software, and the red solid lines denote an empirical light curve. The solid line in the RV plot represents the model for the primary component, and the red dashed line represents the model for the secondary component. |
| Open with DEXTER | |
 |
Fig. A.2
Phase diagrams for B17. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
 |
Fig. A.3
Phase diagrams for MT696. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
 |
Fig. A.4
Phase diagrams for MT720. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
 |
Fig. A.5
Phase diagrams for Schulte 5. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
 |
Fig. A.6
O−C diagram for Schulte 5. Points denote the time difference between the observed times of minimum and the calculated times of minimum using the Pemp and Ṗemp from Table 2. Dashed line shows the O−C value of zero. |
| Open with DEXTER | |
 |
Fig. A.7
Phase diagrams for Schulte 3. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
 |
Fig. A.8
Phase diagrams for MT059. Designations are the same as in Fig. A.1. |
| Open with DEXTER | |
© ESO, 2015
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