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Table 1

Solutions for the incoming asymptotic trajectory (velocity vector) of 2I/Borisov.

Solution α δ v σ(vx) σ(vy) σ(vz) ρ(vx, vy) ρ(vx, vz) ρ(vy, vz)
[deg] [deg] [km s−1] [km s−1] [km s−1] [km s−1]
38 32.79806 59.44090 32.284055 0.0001812 0.0002747 0.0004150 0.8210 0.8735 0.9878
39 32.79823 59.44022 32.284287 0.0003626 0.0003430 0.0005600 0.8465 0.8937 0.9761
40 32.79809 59.44016 32.284313 0.0003774 0.0003438 0.0005601 0.7925 0.8632 0.9725
41 32.79751 59.44008 32.283096 0.0005672 0.0005446 0.0011744 0.8654 0.9090 0.9664
42 32.80272 59.44094 32.279114 0.0006349 0.0003488 0.0011396 0.3297 0.8514 0.6946
43 32.79926 59.43894 32.285134 0.0017506 0.0006598 0.0022294 0.8543 0.9588 0.9173
44 32.79747 59.44015 32.282620 0.0005058 0.0005272 0.0010957 0.8971 0.9430 0.9636
45 32.79747 59.44015 32.282644 0.0004957 0.0005208 0.0010804 0.8989 0.9437 0.9646
46 32.79798 59.44021 32.284561 0.0018604 0.0015284 0.0041306 0.9886 0.9912 0.9925
47 32.79720 59.44014 32.286894 0.0024122 0.0011258 0.0041225 0.9282 0.9886 0.9500

Notes. (α, δ) and v give the barycentric ICRF (International Celestial Reference Frame) direction and asymptotic velocity of 2I/Borisov. σ(vx), σ(vy), σ(vz) are the standard deviations of the Cartesian ICRF velocity components; the last three columns give the correlation coefficients ρ. For orientation, the Galactic coordinates of these solutions are l =132.9°, b = −1.9°. We use only solution 47 in the analysis.

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