Open Access

Fig. 11

image

Dynamical family 179 projected on the proper (sinI, e) plane. The cyan cross indicates the position of the largest member, (179) Klytaemnestra. Most of the family members, more than 300, appear to belong to a clump centered too far from (179) for a physically possible distribution of ejection velocities. Red stars are core family members (with absolute magnitude H < 14, green points are fainter members attached to the core. The members with |z1 | < 0.5 arcsec y−1 are marked by blue circles for core members and blue crosses for attached ones.

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