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Table 1

Time ranges and statistical errors for significant encounters (crossing probability greater than 50%) between the Sun and the Radcliffe wave’s clusters, assuming different threshold distances (dSun–cloud).

dSun–cloud ≤ 50 pc dSun–cloud ≤ 40 pc dSun–cloud ≤ 30 pc dSun–cloud ≤ 20 pc




Name tenter texit tenter texit tenter texit tenter texit
(Myr) (Myr) (Myr) (Myr) (Myr) (Myr) (Myr) (Myr)
Briceno 1 −18.2 ± 0.1 −14.8 ± 0.3 −17.4 ± 0.2 −15.6 ± 0.4
OBP−West −16.3 ±0.3 −13.4 ± 0.3 −15.8 ±0.3 −13.9 ± 0.3
OBP−d −14.2 ± 0.2 −12.2 ± 0.3 −13.6 ± 0.2 −12.6 ± 0.3
Sigma Orionis −13.5 ±0.1 −11.7 ± 0.1
NGC 1980 −15.7 ±0.1 −12.3 ±0.1 −15.3 ±0.1 −12.7 ±0.1 −14.8 ± 0.1 −13.1 ±0.1 −14.3 ±0.1 −13.6 ± 0.2
NGC 1981 −15.0 ± 0.1 −11.7 ± 0.1 −14.7 ± 0.1 −12.0 ± 0.2 −14.3 ± 0.1 −12.4 ± 0.2 −13.9 ± 0.1 −12.8 ±0.2
NGC 1977 −13.4 ± 0.2 −11.5 ± 0.3 −12.8 ±0.2 −11.9 ± 0.3

Radcliffe wave −18.2 ± 0.1 −11.5 ±0.3 −17.4 ± 0.2 −11.9 ± 0.3 −14.8 ± 0.1 −12.4 ± 0.2 −14.3 ±0.1 −12.8 ± 0.2

Notes. This table serves as the numerical complement to Fig. 2.

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