Table 1.
Ejection velocity, galactocentric radius at plane intersection, and stellar mass of the program stars.
| Object | # | vej | rp | M | F |
|---|---|---|---|---|---|
| (km s−1) | (kpc) | (M⊙) | |||
| S5-HVS 1 | 1 |
 |
 |
 |
C |
| B537 | 2 |
 |
 |
 |
D |
| B576 (a) | 3 |
 |
 |
0.5 ± … | C |
| B598 | 4 |
 |
 |
 |
C |
| HVS 5 | 5 |
 |
 |
 |
D |
| HVS 6 | 6 |
 |
 |
 |
R |
| B481 | 7 |
 |
 |
 |
R |
| LAMOST HVS 1 | 8 |
 |
 |
 |
D |
| B434 | 9 |
 |
 |
 |
R |
| LAMOST HVS 2 | 10 |
 |
 |
7.3 ± … | D |
| PG 1610+062 | 11 |
 |
 |
 |
D |
| HVS 7 | 12 |
 |
 |
 |
R |
| LAMOST HVS 4 | 13 |
 |
 |
 |
D |
| J0136+2425 | 14 |
 |
 |
 |
D |
| B733 | 15 |
 |
 |
 |
D |
| B711 | 16 |
 |
 |
 |
R |
| HVS 17 | 17 |
 |
 |
 |
D |
| HVS 8 | 18 |
 |
 |
 |
D |
| B485 | 19 |
 |
 |
 |
D |
| HIP 114569 | 20 |
 |
 |
 |
D |
| PHL 346 | 21 |
 |
 |
 |
D |
| HIP 60350 | 22 |
 |
 |
 |
D |
| EC 04420−1908 | 23 |
 |
 |
 |
D |
| PHL 2018 | 24 |
 |
 |
 |
D |
| LAMOST HVS 3 | 25 |
 |
 |
 |
D |
| B143 | 26 |
 |
 |
 |
D |
| HD 271791 | 27 |
 |
 |
 |
D |
| EC 19596−5356 | 28 |
 |
 |
 |
D |
| BD −2 3766 | 29 |
 |
 |
 |
D |
| HIP 56322 | 30 |
 |
 |
 |
D |
Notes. The given uncertainties are 1σ confidence intervals. The number in the second column is used to identify an object in Fig. 2, Tables A.1 and A.2. The flag in the last column marks objects that potentially originate in the GC (“C”), are bona fide disk runaways (“D”), or stem from the outer rim of the disk (“R”).
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