Volume 403, Number 1, May III 2003
|135 - 140
|Interstellar and circumstellar matter
|29 April 2003
The mass-velocity and intensity-velocity relations in jet-driven molecular outflows
School of Mathematical Sciences, Dublin City University, Dublin 9, Ireland
2 LERMA, Observatoire de Paris, 61 Av. de l'Observatoire, 75014 Paris, France
Corresponding author: T. P. Downes, firstname.lastname@example.org
Accepted: 12 March 2003
We use numerical simulations to examine the mass-velocity and intensity-velocity relations in the CO and H2 S(1)1-0 lines for jet-driven molecular outflows. Contrary to previous expectations, we find that the mass-velocity relation for the swept-up gas is a single power-law, with a shallow slope -1.5 and no break to a steeper slope at high velocities. An analytic bowshock model with no post-shock mixing is shown to reproduce this behaviour very well. We show that molecular dissociation and the temperature dependence of the line emissivity are both critical in defining the shape of the line profiles at velocities above ~20 km s-1. In particular, the simulated CO intensity-velocity relation does show a break in slope, even though the underlying mass distribution does not. These predicted CO profiles are found to compare remarkably well with observations of molecular outflows, both in terms of the slopes at low and high velocities and in terms of the range of break velocities at which the change in slope occurs. Shallower slopes are predicted at high velocity in higher excitation lines, such as H2 S(1)1-0. This work indicates that, in jet-driven outflows, the CO intensity profile reflects the slope of the underlying mass-velocity distribution only at velocities 20 km s-1, and that higher temperature tracers are required to probe the mass distribution at higher speed.
Key words: hydrodynamics / shock waves / ISM: jets and outflows / ISM: molecules
© ESO, 2003
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