Fig. 5: Age-[Fe/H] distributions of the six spatially selected subsamples, colour-coded by birth radius Rbirth.
From: Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars
![Fig. 5: Age-[Fe/H] distributions of the six spatially selected subsamples, colour-coded by birth radius Rbirth.](http://media.springernature.com/full/springer-static/image/art%3A10.1038%2Fs41467-025-56550-1/MediaObjects/41467_2025_56550_Fig5_HTML.png?as=webp)
a–f Arranged according to the division in Fig. 1a. The first row of the figure corresponds to the high-\({{{{\rm{z}}}}}_{\max }\) region, while the second row represents the low-\({{{{\rm{z}}}}}_{\max }\) region. From left to right, the columns depict the inner, local, and outer regions, respectively. As shown in Fig. 1a, high-\({{{{\rm{z}}}}}_{\max }\) refers to \({{{{\rm{z}}}}}_{\max } > \) 0.4 kpc, while low-\({{{{\rm{z}}}}}_{\max }\) indicates \({{{{\rm{z}}}}}_{\max } < \) 0.4 kpc. Inner represents Rguide < 7 kpc, local corresponds to 7 kpc < Rguide < 9 kpc, and outer refers to Rguide > 9 kpc. The numbers of stars in each bin are shown in the top-right corner of each panel. Source data are provided as a Source Data file.
