Table 2.
Accreted stars in our galaxy sample.
| Galaxy name | Maccr, gal (108 M⊙) | faccr, gal (%) | Maccr, thin (108 M⊙) | faccr, thin (%) | Maccr, thick (108 M⊙) | faccr, thick (%) |
|---|---|---|---|---|---|---|
| Au1(1) | 127.5 | 46.1 | – | – | – | – |
| Au2 | 90.7 | 10.7 | 12.0 | 5.4 | 25.7 | 13.9 |
| Au3 | 94.6 | 11.5 | 12.2 | 4.0 | 33.2 | 21.6 |
| Au5 | 40.2 | 6.0 | 7.5 | 5.0 | 19.3 | 29.6 |
| Au6 | 39.5 | 7.8 | 6.4 | 4.1 | 13.0 | 17.6 |
| Au7 | 149.0 | 29.0 | 24.3 | 27.0 | 58.9 | 49.9 |
| Au8 | 51.3 | 15.5 | 10.8 | 13.2 | 26.1 | 16.3 |
| Au9 | 27.8 | 4.6 | 2.0 | 2.9 | 11.3 | 15.8 |
| Au10 | 7.3 | 1.2 | 0.8 | 3.6 | 4.0 | 7.2 |
| Au12 | 88.0 | 14.0 | 22.9 | 12.2 | 42.0 | 55.4 |
| Au14 | 105.3 | 9.9 | 23.7 | 11.2 | 50.9 | 32.4 |
| Au15 | 42.8 | 10.7 | 14.1 | 8.7 | 16.9 | 25.9 |
| Au16 | 41.1 | 6.4 | 13.2 | 4.9 | 22.7 | 15.4 |
| Au17 | 11.4 | 1.5 | 0.9 | 1.6 | 7.6 | 10.2 |
| Au18 | 15.6 | 2.0 | 2.5 | 2.5 | 7.5 | 7.2 |
| Au19 | 98.2 | 18.0 | 22.5 | 12.2 | 31.7 | 26.8 |
| Au21 | 99.1 | 12.7 | 26.3 | 8.3 | 32.5 | 26.6 |
| Au22 | 8.2 | 1.4 | 0.4 | 2.9 | 4.2 | 5.1 |
| Au23 | 56.1 | 6.2 | 4.2 | 4.7 | 27.7 | 19.7 |
| Au24 | 61.3 | 8.5 | 16.6 | 9.1 | 29.5 | 21.6 |
| Au25 | 9.6 | 3.0 | 1.1 | 1.3 | 4.3 | 4.2 |
| Au26 | 117.7 | 10.9 | 3.8 | 5.5 | 48.3 | 24.9 |
| Au27 | 81.4 | 8.5 | 13.7 | 5.8 | 25.9 | 26.4 |
| Au28 | 203.5 | 20.0 | 3.5 | 10.6 | 89.2 | 37.6 |
Notes. Columns from left to right: galaxy name, ex situ mass (mass of accreted stars) in the analyzed region of the galaxy (Maccr, gal), mass fraction of accreted stars in the analyzed region of the galaxy (faccr, gal), ex situ mass in the thin-disk region (Maccr, thin), ex situ mass fraction in the thin-disk region (faccr, thin), ex situ mass in the thick-disk region (Maccr, thick), ex situ mass fraction in the thick-disk region (faccr, thick). (1) Au1 has no clear double disk structure.
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