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Table 5.

Gaia EDR3 proper motion of LMC stars.

Bin α δ d N μαcosδ μδ vϕ
(deg) (deg) (deg) (mas yr−1) (mas yr−1) (km s−1)
1 84.387882 −74.999304 5.19 6084 2.00 ± 0.01 0.56 ± 0.02 36.78 ± 8.62
2 82.192321 −74.600567 4.74 6699 2.05 ± 0.01 0.45 ± 0.02 40.46 ± 8.14
3 86.752693 −74.806033 5.16 5224 1.97 ± 0.01 0.68 ± 0.03 30.00 ± 9.27
4 84.561555 −74.419568 4.64 6099 2.01 ± 0.01 0.58 ± 0.02 36.10 ± 8.64
5 87.154058 −74.212136 4.66 6533 1.95 ± 0.01 0.72 ± 0.02 20.78 ± 8.39
6 90.228859 −74.277969 5.11 5067 1.90 ± 0.02 0.83 ± 0.03 20.55 ± 9.13
7 85.705745 −73.724596 4.06 5330 1.98 ± 0.01 0.65 ± 0.03 24.74 ± 8.27
8 80.645131 −74.078617 4.22 4904 2.05 ± 0.02 0.36 ± 0.03 43.73 ± 9.98
9 88.061728 −73.608670 4.24 5262 1.93 ± 0.02 0.77 ± 0.03 21.36 ± 8.82
10 82.770292 −73.941038 4.09 6460 2.01 ± 0.01 0.48 ± 0.02 32.72 ± 8.80

Notes. Columns (from left to right) refer to the bin number as created by the Voronoi routine, right ascension and declination of the bin centre, angular distance of the bin from the LMC centre, number of stars within each bin, their average proper motion in right ascension and declination, and rotational velocity with respect to the LMC centre. This table is published in its entirety (for all 257 bins) at the CDS. The first ten lines are shown here for guidance regarding its form and content.

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