Early-type stars in the young open cluster NGC 2244 and in the Monoceros OB2 association - I. The multiplicity of O-type stars

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Table 7:

Probability of missing a significant orbital RV variation^a.
Star	M₁	2-10	10-365	365-3000	2-3000
HD 46 056	20.8	0.02	0.17	0.77	0.24
HD 46 149	20.8	0.01	0.04	0.31	0.07
HD 46 150	34.4	0.01	0.03	0.21	0.05
HD 46 202	17.1	0.01	0.09	0.50	0.13
HD 46 223	46.9	0.01	0.03	0.22	0.05
HD 46 485	20.8	0.01	0.20	0.68	0.20
HD 46 573	22.9	0.01	0.06	0.38	0.09
HD 46 966	18.8	0.01	0.06	0.34	0.08
HD 48 279	22.9	0.01	0.07	0.40	0.10

^a Table 7 lists the probability of missing a significant orbital RV variation ( $\Delta {\it RV} > 40$ km s^-1 for the two rapid rotators and $\Delta RV > 20$ km s^-1 for the other stars). M₁ represents the primary mass and is expressed in $M_{\odot}$ . The last four columns are classified according to the orbital period of the system (in days).

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