Table 1
List of candidate cluster positions, apparent radii, ⟨AKs⟩, and modulus distances (DM).
ID | RA(J2000)a | Dec(J2000)a | radius | ⟨ AKs field ⟩ b | DM(⟨ AKs field ⟩ )c | ⟨ AKs cRSGs ⟩ d | DM(⟨ AKs RSGs ⟩)e | DM(red clump)f | DM(Sp)g |
[ hh mm ss ] | [°′′′] | [′′] | [ mag ] | [ mag ] | [ mag ] | [ mag ] | [ mag ] | [ mag ] | |
|
|||||||||
cl1.5 | 17 53 45.09 | –28 11 08.29 | 73 | 0.45 ± 0.08 | (12.7 ± 0.2) | ··· | ··· | 14.54 ± 0.16 | ··· |
cl9.5 | 18 10 54.34 | –21 12 37.67 | 60 | 0.70 ± 0.11 | (13.3 ± 0.2) | ··· | ··· | 14.05 ± 0.12 | ··· |
cl16.7 | 18 23 34.40 | –14 39 10.86 | 76 | 0.44 ± 0.27 | 12.7 ± 0.9 | 0.49 ± 0.03 | 12.8 ± 0.1 | 12.93 ± 0.13 | ··· |
cl49.3 | 19 19 31.53 | 14 54 08.57 | 130 | 0.48 ± 0.35 | 13.8 ± 1.9 | 0.47 ± 0.11 | 13.7 ± 0.5 | 14.22 ± 0.12 | 14.16 ± 1.00 |
cl59.8 | 19 46 18.57 | 23 22 30.23 | 85 | 0.26 ± 0.17 | 12.9 ± 1.4 | ··· | ··· | ··· | ··· |
Notes.
⟨ AKs field ⟩ is the average AKs of the spectroscopically observed late-type stars in the field.
DM(⟨ AKs field ⟩) is the distance modulus obtained from the AKs values of detected late-type stars and the model of Drimmel et al. (2003).
DM(⟨ AKs RSGs ⟩) is the distance modulus obtained from the AKs values of cRSGs and the model of Drimmel et al. (2003).
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