Issue |
A&A
Volume 577, May 2015
|
|
---|---|---|
Article Number | A11 | |
Number of page(s) | 27 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201425475 | |
Published online | 23 April 2015 |
Online material
Fig. 21
LiIEW vs. I magnitude or CoRoT counts. |
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Open with DEXTER |
Fig. 22
Spitzer IRAC 3.6 μm and 4.5 μm light curves (blue and red filled circles, respectively) overplotted on CoRoT light curves (black circles). The CoRoT and IRAC 3.6 μm light curves were shifted in magnitude for easier comparison. |
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Open with DEXTER |
Fig. 22
continued. |
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Open with DEXTER |
Fig. 23
Simulated light curves of AA Tau-like stars (red) plotted over CoRoT light curves (black). |
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Open with DEXTER |
Fig. 24
I-band or CoRoT light curves and u − r color diagrams folded in phase. |
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Open with DEXTER |
Fig. 24
continued. |
|
Open with DEXTER |
© ESO, 2015
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