2001ApJ...552L.167Z

A survey for molecular outflows was carried out by mapping the CO J=2-1 line toward a sample of 69 luminous IRAS point sources. Sixty objects have IRAS luminosities from 10³ to 10⁵ L_☉ and are associated with dense gas traced by NH₃, identifying them as high-mass star-forming regions. Among 69 sources, 65 sources have data that are suitable for outflow identification. Thirty-nine regions show spatially confined high-velocity wing emission in CO, indicative of molecular outflows. Most objects without identifiable outflows lie within 0°<l<50° where outflow signatures are confused by multiple cloud components along the line of sight. Excluding 26 sources with 0°<l<50°, we found 35 outflows out of 39 sources, which yields an outflow detection rate of 90%. Many of the outflows contain masses of more than 10 M_☉ and have momenta of a few hundred M_☉ km.s^–1, at least 2 orders of magnitude larger than those in typical low-mass outflows. This class of massive and energetic outflows is most likely driven by high-mass young stellar objects. The high detection rate indicates that molecular outflows are common toward high-mass young stars. Given the connection between outflows and accretion disks in low-mass stars, we suggest that high-mass stars may form via an accretion-outflow process, similar to their low-mass counterparts.