Table 4
Comparison of encounter parameters with those reported by Kalas et al. (2001).
| Hipparcos ID | Gaia DR3 ID | Encounter time (Myr) | Encounter distance (pc) | Encounter velocity (km s−1) | |||
|---|---|---|---|---|---|---|---|
| Kalas et al. | This work | Kalas et al. | This work | Kalas et al. | This work | ||
| 10798 | 5117974602912370432 | ![]() |
![]() |
![]() |
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42.8 ± 1.3 | 40.2 ± 0.4 |
| 17378 | 5164120762333028736 | ![]() |
![]() |
![]() |
![]() |
47.9 ± 1.5 | 45.0 ± 0.5 |
| 19893 | 4781833626056162688 | ![]() |
![]() |
![]() |
![]() |
13.4 ± 1.4 | 14.8 ± 0.8 |
| 19921 | 46786647663938295041 | ![]() |
![]() |
![]() |
![]() |
28.6 ± 0.6 | 29.8 ± 0.3 |
| 22122 | 47848050562305873922 | ![]() |
![]() |
![]() |
![]() |
62.7 ± 1.5 | 62.3 ± 0.2 |
| 23693 | 47639068792394616321 | ![]() |
![]() |
![]() |
![]() |
21.6 ± 1.5 | 18.0 ± 0.5 |
| 25544 | 4759543295545939840 | ![]() |
![]() |
![]() |
![]() |
25.5 ± 0.9 | 24.5 ± 0.2 |
| 27628 | 2887731882922767744 | ![]() |
![]() |
![]() |
![]() |
83.9 ± 2.1 | 87.0 ± 1.3 |
| 29568 | 29134111831496157441 | ![]() |
![]() |
![]() |
![]() |
11.6 ± 0.5 | 10.1 ± 0.2 |
| 29958 | 2993676867708999296 | ![]() |
![]() |
![]() |
![]() |
102.1 ± 5.6 | 97.4 ± 0.8 |
| 31711 | 54797787652785895682 | ![]() |
![]() |
![]() |
![]() |
14.6 ± 1.4 | 17.5 ± 1.2 |
| 37504 | 5263150888430619904 | ![]() |
![]() |
![]() |
![]() |
37.6 ± 1.5 | 40.5 ± 0.4 |
| 38908 | 52910281811198517761 | ![]() |
![]() |
![]() |
![]() |
49.5 ± 0.8 | 48.1 ± 0.2 |
| 83990 | 5914096303621755520 | ![]() |
![]() |
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60.4 ± 1.5 | 57.0 ± 0.4 |
| 89042 | 66340327405442360322 | ![]() |
![]() |
![]() |
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50.6 ± 1.6 | 48.3 ± 0.3 |
| 114996 | 64924067437069077762 | ![]() |
![]() |
![]() |
![]() |
29.3 ± 0.8 | 22.7 ± 0.7 |
| 116250 | 6353376831270492800 | ![]() |
![]() |
![]() |
![]() |
22.9 ± 1.7 | 23.9 ± 0.3 |
Notes. The first two columns list the HIPPARCOS IDs and the corresponding GDR3 IDs. To compare with Kalas et al. (2001) results, we computed time-distance uncertainties as the limits of the 2D 1σ contours (39.35%), based on Mahalanobis distances. Velocity uncertainties are given as 1σ intervals of the marginal distributions (13.6th–86.4th percentiles). The full table is available on Zenodo. (1)According to SIMBAD, this star belongs to a binary or multiple system. (2)This HIPPARCOS-Gaia identification was taken from SIMBAD, as it is not present in the Gaia Archive crossmatch tables.
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