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This is the second paper of the statistical study of coronal mass ejection(CME) source locations, in which the relationship between CMEs and activeregions (ARs) is statistically studied on the basis of the information of CMEsource locations and the ARs automatically extracted from magnetic synopticcharts of Michelson Doppler Imager (MDI) during 1997 -- 1998. It is found thatabout 63% of the CMEs are related with ARs, at least about 53% of the ARsproduced one or more CMEs, and particularly about 14% of ARs are CME-rich (3 ormore CMEs were generated) during one transit across the visible disk. Severalissues are then tried to clarify: whether or not the CMEs originating from ARsare distinct from others, whether or not the CME kinematics depend on ARproperties, and whether or not the CME productivity depends on AR properties.The statistical results suggest that (1) there is no evident difference betweenAR-related and non-AR-related CMEs in terms of CME speed, acceleration andwidth, (2) the size, strength and complexity of ARs do little with thekinematic properties of CMEs, but have significant effects on the CMEproductivity, and (3) the sunspots in all the most productive ARs at leastbelong to $\beta\gamma$ type, whereas 90% of those in CME-less ARs are $\alpha$or $\beta$ type only. A detailed analysis on CME-rich ARs further reveals that(1) the distribution of the waiting time of same-AR CMEs, consists of two partswith a separation at about 15 hours, which implies that the CMEs with a waitingtime shorter than 15 hours are probably truly physical related, and (2) an ARtends to produce such related same-AR CMEs at a pace of 8 hours, but cannotproduce two or more fast CMEs (>800 km/s) within a time interval of 15 hours.This interesting phenomenon is particularly discussed.

Statistical Study of Coronal Mass Ejection Source Locations: II. Role of Active Regions in CME Production