Issue |
A&A
Volume 539, March 2012
|
|
---|---|---|
Article Number | A125 | |
Number of page(s) | 21 | |
Section | Galactic structure, stellar clusters and populations | |
DOI | https://doi.org/10.1051/0004-6361/201118206 | |
Published online | 06 March 2012 |
Online material
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Fig. 3
Graphs for the filtering of open cluster NGC 2477. Upper graphs give all UBV data and lower ones the filtered and weighted data and the fitted isochrone and ZAMS (solid lines). The symbol size is proportional to likelihood value. |
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Fig. 4
Graphs for the filtering of open cluster NGC 2477. Upper graphs give all 2MASS data and lower ones the filtered and weighted data and the fitted isochrone and ZAMS (solid lines). The symbol size is proportional to likelihood value. |
Open with DEXTER |
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Fig. 9
Same as Fig. 1 for Berkeley 32. |
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Fig. 10
Same as Fig. 2 for Berkeley 32. |
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Fig. 21
Same as Fig. 1 for Melotte 105 (Ref. 289). |
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Fig. 22
Same as Fig. 1 for Melotte 105 (Ref. 32). |
Open with DEXTER |
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Fig. 23
Same as Fig. 2 for Melotte 105. |
Open with DEXTER |
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Fig. 24
Same as Fig. 1 for Trumpler 1 (Ref. 86). |
Open with DEXTER |
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Fig. 25
Same as Fig. 1 for Trumpler 1 (Ref. 320). |
Open with DEXTER |
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Fig. 26
Same as Fig. 2 for Trumpler 1. |
Open with DEXTER |
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Fig. 29
Comparison of our fit with that of Bica et al. (2004) for Dias 6. See the text for details. |
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Fig. 30
Comparison of our fit with that of Tadross (2008) for Dias 6. See the text for details. |
Open with DEXTER |
© ESO, 2012
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