New BVRI photometry results on Kuiper Belt Objects from the ESO VLT

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Table 6:

Object summary.
			Types
	All	Classic	Cold	Hot	SDOs	Cent
This work	30	19	9	10	10 $^{(\star)}$	1
LP	53	33	16	17	10	10 $^{(\bullet)}$
2MS	33	21	6	15	5	7
Total	116	73	31	42	25	18

Number of objects for the different dynamical groups (except the 2 Neptune's resonant objects): All (the whole sample), Classic (classical TNOs), Cold (classical TNOs with inclinations < $4.5^{\circ}$ ), hot (classical TNOs with inclinations > $4.5^{\circ}$ ), SDOs (scattered disk objects), and Cent (Centaurs). LP is the ESO Large Program (Boehnhardt et al. 2002; Peixinho et al. 2004), and 2MS the Meudon Multicolor Survey (Doressoundiram et al. 2005). $^{(\star)}$ We include the peculiar distant object 2000CR₁₀₅. $^{(\bullet)}$ We include the uncertain Centaur 2002CB₂₄₉.

Source LaTeX | All tables | In the text

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