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Table 5

Results of the kinematic investigation of HE 0437-5439.

Run Model I Model II Model III



dp (kpc) Tp (Myr) vp (km s-1) dp (kpc) Tp (Myr) vp (km s-1) dp (kpc) Tp (Myr) vp (km s-1)

#1a 13.2 ± 4.5 −22 ± 13 640 ± 70 13.2 ± 4.5 −22 ± 13 640 ± 70 13.1 ± 4.4 −22 ± 13 640 ± 70
#1b 15.6 ± 10.4 −98 ± 15 690 ± 50 15.7 ± 10.3 −98 ± 16 680 ± 50 14.8 ± 10.1 −95 ± 14 730 ± 40
#2 11.0 ± 4.5 −23 ± 12 680 ± 80 10.9 ± 4.5 −23 ± 12 680 ± 80 11.0 ± 4.5 −23 ± 12 680 ± 80
#3a 7.5 ± 3.6 −26 ± 11 680 ± 80 7.5 ± 3.7 −26 ± 12 680 ± 80 7.6 ± 3.7 −26 ± 12 680 ± 80
#3b 16.6 ± 8.6 −95 ± 12 690 ± 30 17.0 ± 8.9 −95 ± 12 690 ± 30 15.8 ± 8.5 −93 ± 12 730 ± 20

Notes.dp is the distance, Tp the time, and vp the relative velocity at periastron of HE 0437-5439 with respect to the center of the LMC (runs #1a, #2, and #3a) or to the GC (runs #1b and #3b). Numbers are mean value ± standard deviation σ. The initial conditions of runs #1 are those of Brown et al. (2010). In runs #2 and #3a, Kroupa & Bastian’s (1997) LMC proper motions are used. In runs #3, proper motions of HE 0437-5439 are increased by their systematic errors (CTI correction, see text for details).

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