Table 6.
Distances (in kpc) for distance indicator Miras.
| ID | DBEAM | DSurot | DJKs |
DHKs |
||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (C89) | (N06) | (N09) | (AG17) | (D19) | (S20) | (C89) | (N06) | (N09) | (AG17) | (D19) | ||||
| 302108018024 | 152.8 | 154.0 | ||||||||||||
| 305410041654 | 586.8 | 584.1 | ||||||||||||
| 307102042261 | 253.7 | 258.0 | ||||||||||||
| 307304149161 | 198.8 | 200.4 | ||||||||||||
| 307408087155 | 144.0 | 144.2 | ||||||||||||
| 308616154874 | 344.6 | 343.0 | ||||||||||||
| 309203069542 | 150.3 | 153.6 | ||||||||||||
| 309209099809 | 140.4 | 139.9 | 77.8 | 96.2 | 91.6 | 103.2 | 92.6 | 104.7 | 78.8 | 84.2 | 72.3 | 94.9 | 79.2 | |
| 309304135416 | 206.3 | 204.8 | ||||||||||||
| 319213010190 | 132.9 | 118.7 | ||||||||||||
| 319302072957 | 53.2 | 51.0 | 5.2 | 6.9 | 3.7 | 11.2 | 5.4 | |||||||
| 319509072340 | 59.1 | 48.3 | 4.7 | 6.1 | 3.3 | 10.0 | 4.8 | |||||||
| 320106023807 | 70.8 | 75.5 | 35.9 | 50.4 | 46.6 | 56.3 | 47.4 | 57.7 | 37.1 | 41.2 | 32.4 | 49.9 | 37.5 | |
| 320201006873 | 50.8 | 49.6 | 4.3 | 5.7 | 2.9 | 9.6 | 4.4 | |||||||
| 320201014922 | 51.9 | 45.9 | 4.6 | 6.1 | 3.2 | 10.2 | 4.7 | |||||||
| 320201073554 | 108.4 | 88.4 | 10.7 | 13.8 | 7.8 | 21.5 | 11.0 | |||||||
| 320515091949 | 175.9 | 175.3 | ||||||||||||
| 364104082076 | 162.3 | 165.1 | ||||||||||||
Notes. For each nonsaturated star in our sample of distance indicator Miras (whose IDs are shown in Col. (1)), distance values (in kpc) are given on the basis of the apparent distance moduli in Ks, corrected (in each case) according to the extinction values given in Table 5. We note that, as explained in the text, the distances derived on the basis of the BEAM and Surot extinction maps, for stars located beyond the Galactic bulge, should be considered as upper limits only.
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