EDP Sciences
Free Access
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.1A.8 show individual data sets together with the phased model curves.

thumbnail Fig. A.1

Phase diagrams for A36 using the Pemp and emp 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.

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thumbnail Fig. A.2

Phase diagrams for B17. Designations are the same as in Fig. A.1.

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thumbnail Fig. A.3

Phase diagrams for MT696. Designations are the same as in Fig. A.1.

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thumbnail Fig. A.4

Phase diagrams for MT720. Designations are the same as in Fig. A.1.

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thumbnail Fig. A.5

Phase diagrams for Schulte 5. Designations are the same as in Fig. A.1.

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thumbnail Fig. A.6

OC 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 emp from Table 2. Dashed line shows the OC value of zero.

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thumbnail Fig. A.7

Phase diagrams for Schulte 3. Designations are the same as in Fig. A.1.

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thumbnail Fig. A.8

Phase diagrams for MT059. Designations are the same as in Fig. A.1.

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© ESO, 2015

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