Issue |
A&A
Volume 437, Number 2, July II 2005
|
|
---|---|---|
Page(s) | 517 - 524 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361:20042253 | |
Published online | 21 June 2005 |
Long-duration simulations of the evolution of jet-driven molecular outflows
School of Mathematical Sciences, Dublin City University, Glasnevin, Dublin 9, Ireland e-mail: turlough.downes@dcu.ie
Received:
26
October
2004
Accepted:
22
March
2005
We use numerical simulations to examine the mass-velocity, , and
intensity-velocity,
, relations in jet-driven molecular outflows up to
an age of 2300 yr. We find that the
relation is a power-law,
, the exponent of which increases with time up to
at
yr. It then becomes roughly
constant. This indicates that γ does not evolve throughout the
lifetime of a molecular outflow, at least in the context of the jet-driven
model.
We also investigate the effect of long-period episodicity of the jet on the
and
relations. We find that, contrary to previous expectations,
these relations are not significantly changed with the introduction of
such variability into the jet.
Finally, we present a novel, and relatively simple, parallelisation method
for the code used in these simulations. This gives an increase of
roughly a factor of 4 in speed over standard methods, and allows the
simulations presented here to be run fairly easily, even with modest
computational resources.
Key words: hydrodynamics / shock waves / ISM: jets and outflows / ISM: molecules
© ESO, 2005
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