We present observations of outflows in the star-forming region NGC 1333 using the Combined Array for Research in Millimeter-Wave Astronomy ( CARMA ) .
We combined the ^ { 12 } CO and ^ { 13 } CO ( 1-0 ) CARMA mosaics with data from the 14-m Five College Radio Astronomy Observatory ( FCRAO ) to probe the central , most dense and active region of this protostellar cluster at scales from 5 ^ { \prime \prime } to 7 ^ { \prime } ( or 1000 AU to 0.5 pc at a distance of 235 pc ) .
We map and identify ^ { 12 } CO outflows , and along with ^ { 13 } CO data we estimate their mass , momentum and energy .
Within the 7 ^ { \prime } \times 7 ^ { \prime } map , the 5 ^ { \prime \prime } resolution allows for a detailed study of morphology and kinematics of outflows and outflow candidates , some of which were previously confused with other outflow emission in the region .
In total , we identify 22 outflow lobes , as well as 9 dense circumstellar envelopes marked by continuum emission , of which 6 drive outflows .
We calculate a total outflow mass , momentum and energy within the mapped region of 6 M _ { \odot } , 19 M _ { \odot } km s ^ { -1 } , and 7 \times 10 ^ { 44 } erg , respectively .
Within this same region , we compare outflow kinematics with turbulence and gravitational energy , and we suggest that outflows are likely important agents for the maintenance of turbulence in this region .
In the earliest stages of star formation , outflows do not yet contribute enough energy to totally disrupt the clustered region where most star formation is happening , but have the potential to do so as the protostellar sources evolve .
Our results can be used to constrain outflow properties , such as outflow strength , in numerical simulations of outflow-driven turbulence in clusters .