Fig. 2
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Main-belt asteroid distributions in (a, i) space. Gray dots show objects from the Minor Planet Center database and red dots show the selected sample. Dotted black lines mark the twenty most populated three-body MMRs from Table 2: (1) 4J-2S-1, (2) 2M+2J-5, (3) 2M-7J-2, (4) 2J+2S-1, (5) 6J-1S-2, (6) 4J-3S-1, (7) 3M-5J-5, (8) 1M-9J+1, (9) 1M-9S-1, (10) 1J-9S-1, (11) 2M-10J-1, (12) 1J+4S-1, (13) 5J+7S-3, (14) 3J-1S-1, (15) 1J+3S-1, (16) 3J-2S-1, (17) 5J-7S-1, (18) 1M-2J-2, (19) 1M-5S-2, and (20) 5J-2S-2. Blue vertical lines indicate five most important Kirkwood gaps in this region.
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