| Issue |
A&A
Volume 569, September 2014
|
|
|---|---|---|
| Article Number | A13 | |
| Number of page(s) | 26 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201423415 | |
| Published online | 10 September 2014 | |
Online material
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Fig. 8
Residuals of star density in colour magnitude diagrams for 9 2MASS fields for the model with a single star formation episode. The longitude and latitude of each field considered are indicated in each panel. The residuals are indicated in the colour level and in contours that are labelled with their level. |
| Open with DEXTER | |
 |
Fig. 9
Residuals of star density in colour magnitude diagrams for 9 SDSS fields for the model with a single star formation episode. The longitude and latitude of each field considered are indicated in each panel. The residuals are indicated in the colour level and in contours that are labelled with their level. |
| Open with DEXTER | |
 |
Fig. 10
Residuals of star density in colour magnitude diagrams for 9 2MASS fields for the model with two episodes of star formation in the thick disc. The longitude and latitude of each field considered are indicated in each panel. The residuals are indicated in the colour level and in contours that are labelled with their level. |
| Open with DEXTER | |
 |
Fig. 11
Residuals of star density in colour magnitude diagrams for 9 SDSS fields for the model with two episodes of star formation in the thick disc. The longitude and latitude of each field considered are indicated in each panel. The residuals are indicated in the colour level and in contours that are labelled with their level. |
| Open with DEXTER | |
© ESO, 2014
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