Table 7
Parameters of the bow-shock candidates and medium density.
| Source | l | w | R | l | w | R | n ISM | Source | l | w | R | l | w | R | n ISM | ||||||||||||||||
| [′] | [pc] | [cm-3] | [′] | [pc] | [cm-3] | ||||||||||||||||||||||||||
|
|
|||||||||||||||||||||||||||||||
| HIP 44368 | 5 | 1.25 | 0.8 | 2.76 | 0.69 | 0.44 | 1.8 | G1 | 4 | 0.8 | 0.8 | 1.98 | 0.4 | 0.4 | 14 | ||||||||||||||||
| HIP 46928 | 1.8 | 0.47 | 1 | 0.09 | 0.02 | 0.05 | 2 | G2 | 6 | 1.2 | 1.2 | 2.97 | 0.59 | 0.59 | 14 | ||||||||||||||||
| HIP 47868 | 5 | 1.7 | 1.6 | 1.56 | 0.53 | 0.50 | 2.6 | G3 | 5 | 1.5 | 1 | 2.47 | 0.74 | 0.49 | 16 | ||||||||||||||||
| HIP 98418 | 1.66 | 0.6 | 0.5 | 0.26 | 0.09 | 0.08 | 380 | G4 | 3 | 1 | 0.8 | 1.48 | 0.49 | 0.4 | 42 | ||||||||||||||||
| HIP 101186* | 22 | 4 | 4.5 | 9.50 | 1.73 | 1.94 | 2.63 | G5 | 3 | 1 | 1 | 1.48 | 0.49 | 0.49 | 4 | ||||||||||||||||
| HIP 104579 | 3 | 1.3 | 1.1 | 1.00 | 0.43 | 0.37 | 0.7 | G6 | 1.5 | 0.5 | 0.4 | 0.74 | 0.25 | 0.2 | 13 | ||||||||||||||||
| HIP 105186 | 7 | 2 | 2.5 | 2.30 | 0.66 | 0.82 | 0.3 | G7 | 1.5 | 0.5 | 0.3 | 0.74 | 0.25 | 0.15 | 23 | ||||||||||||||||
| HIP 107789 | 1.2 | 0.4 | 0.3 | 0.42 | 0.14 | 0.10 | 1.8 | G8 | 1.5 | 0.5 | 0.5 | 0.74 | 0.25 | 0.25 | 5 | ||||||||||||||||
| BD +43° 3654* | 19 | 3 | 4 | 8.01 | 1.26 | 1.69 | 3.5 | 4U 1907+09 | 3.5 | 1 | 1.5 | 4.07 | 1.16 | 1.74 | 0.1 | ||||||||||||||||
| HD 57682 | 1.6 | 0.4 | 0.3 | 0.74 | 0.19 | 0.14 | 85 | J1117-6120 | 1.5 | 0.5 | 0.5 | 3.31 | 1.1 | 1.1 | 6.4 | ||||||||||||||||
| HIP 86768 | 4 | 2 | 2 | 0.86 | 0.43 | 0.43 | 0.1 | BD −14 5040 | 4 | 1 | 1 | 2.09 | 0.52 | 0.52 | 0.1 | ||||||||||||||||
| RCW 49-S1 | 2.5 | 0.5 | 0.7 | 4.43 | 0.89 | 1.24 | 30 | Star 1 | 7 | 1 | 1.5 | 3.66 | 0.52 | 0.78 | – | ||||||||||||||||
| K1 | 3 | 1 | 0.7 | 1.31 | 0.44 | 0.31 | 4 | SER1 | 4 | 1.5 | 1 | – | – | – | – | ||||||||||||||||
| K2 | 4 | 0.3 | 0.5 | 1.74 | 0.13 | 0.22 | 1.7 | SER2 | 2.5 | 1 | 1 | – | – | – | – | ||||||||||||||||
| K3 | 2 | 0.5 | 0.4 | 0.87 | 0.22 | 0.17 | 16.6 | SER3 | 2.5 | 0.5 | 0.5 | – | – | – | – | ||||||||||||||||
| K4 | 1 | 0.3 | 0.3 | 0.44 | 0.13 | 0.13 | 2.8 | SER4 | 2.5 | 1 | 1 | – | – | – | – | ||||||||||||||||
| K5 | 4 | 1 | 1 | 1.74 | 0.44 | 0.44 | 2 | SER5 | 6 | 1 | 2 | – | – | – | – | ||||||||||||||||
| K6 | 2.5 | 0.5 | 0.7 | 1.09 | 0.22 | 0.31 | 0.4 | SER6 | 2.5 | 0.6 | 0.5 | – | – | – | – | ||||||||||||||||
| K7 | 5 | 1 | 1.5 | 2.18 | 0.44 | 0.65 | 44 | SER7 | 8 | 1.5 | 1.5 | – | – | – | – | ||||||||||||||||
| K10 | 2 | 0.5 | 0.5 | 0.87 | 0.22 | 0.22 | 1.8 | ||||||||||||||||||||||||
Notes. Columns 2 to 4 and 10 to 12: length l and width w of the bow-shock structure, and distance R from the star to the midpoint of the bow shock, in angular units. The sizes were estimated from WISE band 4 (22 μm) images, and with band 3 (12.1 μm) images when identification was not clear in band 4. Columns 5 to 7 and 13 to 15: same variables as before, in linear units, for those stars of known distances. Columns 8 and 16: ambient density as derived in Peri et al. (2012; Wilkin 1996).
Studied in E-BOSS r1 (Peri et al. 2012) only through MSX images.
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