Free Access
Issue
A&A
Volume 549, January 2013
Article Number A86
Number of page(s) 8
Section Stellar structure and evolution
DOI https://doi.org/10.1051/0004-6361/201220562
Published online 03 January 2013

Online material

PDF file of pages 9 to 28 (21.48 MB) (Access here)

PDF file of pages 29 to 47 (32.58 MB) (Access here)

Table 1

Period and period change determinations for 143 eclipsing binary candidates.

thumbnail Fig. 12

Folded lightcurves (left) and O−C diagrams (right) for 143 objects. On the O−C diagrams, the dotted lines represent the best linear fit to the data, and the solid lines the best quadratic fit. Note that many O−C diagrams represent non-significant period change, or were disregarded due to paucity of data: see Table 1 for significant results.

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© ESO, 2013

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