EDP Sciences
Free Access
Issue
A&A
Volume 545, September 2012
Article Number A5
Number of page(s) 12
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201219467
Published online 28 August 2012

Online material

Appendix A: Individual angular diameter determinations

We present here the different individual LD angular diameter determinations for the various epochs of observation of θ Cygni. The individual LD diameters are given in Table 11.

thumbnail Fig. A.1

Model of squared visibility for the RJD 55 849.62 (left, θLD = 0.700 ± 0.011) and 55 848.62 (right, θLD = 0.744 ± 0.007) obtained by LITpro.

Open with DEXTER

thumbnail Fig. A.2

Model of squared visibility for the RJD 55 826.67 (left, θLD = 0.721 ± 0.009) and 55 805.75 (right, θLD = 0.727 ± 0.010) obtained by LITpro.

Open with DEXTER

thumbnail Fig. A.3

Model of squared visibility for the RJD 55 803.77 (left, θLD = 0.759 ± 0.008) and 55 774.73 (right, θLD = 0.807 ± 0.010) obtained by LITpro.

Open with DEXTER

thumbnail Fig. A.4

Model of squared visibility for the RJD 55 722.93 (left, θLD = 0.793 ± 0.006) and 55 486.71 (right, θLD = 0.744 ± 0.007) obtained by LITpro.

Open with DEXTER

thumbnail Fig. A.5

Model of squared visibility for the RJD 55 370.92 (θLD = 0.764 ± 0.010) obtained by LITpro.

Open with DEXTER


© ESO, 2012

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