Discovery of an extremely wide-angle bipolar outflow in afgl 5142

Most bipolar outflows are associated with individual young stellar objects and have small opening angles. Here we report the discovery of an extremely wide-angle (similar to 180 degrees) bipolar outflow ("EWBO") in a cluster forming region AFGL 5142 from low-velocity emission of the HCN (3-2) and HCO+ (3-2) lines. This bipolar outflow is along a north-west to south-east direction with a line of sight flow velocity of about 3 km s(-1) and is spatially connected to the high-velocity jet-like outflows. It seems to be a collection of low-velocity material entrained by the high-velocity outflows due to momentum feedback. The total ejected mass and mass loss rate due to both high-velocity jet-like outflows and the "EWBO" are similar to 24.5 M-circle dot and similar to 1.7 x 10(-3)M(circle dot) yr(-1), respectively. Global collapse of the clump is revealed by the " blue profile" in the HCO+ (1-0) line. A hierarchical network of filaments was identified in NH3 (1, 1) emission. Clear velocity gradients of the order of 10 km s(-1) pc(-1) are found along filaments, indicating gas inflow along the filaments. The sum of the accretion rate along filaments and mass infall rate along the line of sight is similar to 3.1 x 10(-3) M-circle dot yr(-1), which exceeds the total mass loss rate, indicating that the central cluster is probably still gaining mass. The central cluster is highly fragmented and 22 condensations are identified in 1.1 mm continuum emission. The fragmentation process seems to be determined by thermal pressure and turbulence. The magnetic field may not play an important role in fragmentation.Chinese Academy of Sciences, Science and Technology Facilities Council of the United Kingdom, KASI fellowship, China Ministry of Science and Technology under State Key Development Program for Basic Research, NSFC, Top Talents Program of Yunnan Province, ESO fellowship, Basic Science Research Program through the National Research Foundation of Korea (NRF) - Ministry of Education, Science, and Technology, global research collaboration of Korea Research Council of Fundamental Science & Technology (KRCF), Basic Science Research Program through the National Research Foundation of Korea (NRF), Korea Astronomy and Space Science Institute under the RD progra