A single distance sample of molecular outflows from high-mass young stellar objects

¹ Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD, UK
² : FCRAO, 619 Lederle Graduate Research Center, University of Massachusetts, Amherst, MA 01003, USA

Corresponding author: N. A. Ridge, naomi@fcrao.umass.edu

Received: 11 June 2001
Accepted: 22 August 2001

Abstract

We have made ¹²CO 2-1 and 1-0 maps of eleven molecular outflows associated with intermediate to high-mass young stellar objects (YSOs) in order to establish whether the correlations between outflow parameters and source bolometric luminosity hold in the high-mass regime. It is important to consider the effects of Malmquist-type biases when looking at high-mass YSOs, as they are generally much more distant than their low mass counterparts. We therefore chose only objects located at ~2 kpc. We find that the relations show much more scatter than is seen in similar studies of low-mass YSOs. We also find that the mass-spectrum is significantly steeper in high-mass outflows, indicating a larger mass-fraction at lower velocities, a low collimation factor (~1-2) and no Hubble-like relationship.