Fig. 10.
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Three-colour image of NGC 1850, created from HST observations in the F336W (blue), F438W (green) and F814W (red) filters. Member stars of NGC 1850 are selected based on their motion and distance from the cluster centre (white solid circle). Stars belonging to the young group called NGC 1850B are selected as the young sequence in the CMD that are located within the white dashed circle and show consistent motions.Three-colour image of NGC 1850, created from HST observations in the F336W (blue), F438W (green) and F814W (red) filters. Member stars of NGC 1850 are selected based on their motion and distance from the cluster centre (white solid circle). Stars belonging to the young group called NGC 1850B are selected as the young sequence in the CMD that are located within the white dashed circle and show consistent motions.
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