Jet-Accelerated Molecular Outflows: The Mass-Velocity and Intensity-Velocity Relations

Details Jet-Accelerated Molecular Outflows: The Mass-Velocity and Intensity-Velocity Relations Jet-Accelerated Molecular Outflows: The Mass-Velocity and Intensity-Velocity Relations

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..120d&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Ism: Jets And Outflows, Stars: Mass Loss, Stars: Pre-Main Sequence

Scientific paper

We use numerical simulations to clarify the mass-velocity and intensity-velocity relations for jet-driven outflows. The simulated CO profiles reproduce the broken power laws observed of molecular outflows remarkably well, with no need for two distinct entrainment regimes. An analytic model is proposed to explain the exponent =~ - 1.5 of the underlying smooth mass-velocity relation.

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