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Table 2.

Arches found at small scale j = 3 (4–8 km s−1).

n. Contains Start (VR, Vϕ) End (VR, Vϕ) 0-cross Reduced χ2
A1 136.5, −254.5 −136.5, −255.0 −293.4 4.09
A2 21.5, −276.5 −17.5, −279.0 −276.4 1.20
A3 γ Leo −47.5, −260.5 −100.0, −239.5 −246.5 335.05
A4 Sirius 129.0, −238.0 −58.5, −244.0 −258.4 25.52
A5 Coma, Dehnen98-6 −0.5, −246.5 −29.5, −230.0 −246.5 44.96
A6 Dehnen98-14 −53.0, −228.0 −73.5, −222.0 −200.4 1290.04
A7 Hyades, Pleiades 51.0, −233.0 −103.5, −183.5 −227.7 111.01
A8 117.0, −201.5 10.0, −212.0 −209.1 297.48
A9 Hercules, ϵInd 70.5, −204.0 −71.5, −180.0 −201.9 42.84
A10 HR 1614 21.5, −185.5 −33.5, −182.5 −188.3 1.14
A11 Bobylev 16-22 90.0, −177.0 46.0, −179.0 −203.7 260.49
A12 Arcturus 45.0, −155.5 −31.0, −149.5 −159.2 5.50

Notes. The arches are those appearing in Fig. 3, ordered by increasing Vϕ. For each arch we give a label in the first column, the Classical MGs that it contains (if any) in the second column, and three of its points in the velocity plane in Cols. 3–5, that is, the coordinates of the first and last peak of the line, and the expected azimuthal velocity corresponding to zero radial velocity, respectively. The last column shows a reduced χ2 between the arch and the corresponding track of constant kinetic energy.

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