A highly-collimated SiO jet in the HH212 protostellar outflow

Details A highly-collimated SiO jet in the HH212 protostellar outflow A highly-collimated SiO jet in the HH212 protostellar outflow

2006-12-18

arxiv.org/abs/astro-ph/0612482v1

Astronomy and Astrophysics

Astrophysics

Astronomy and Astrophysics Letter, in press

Scientific paper

10.1051/0004-6361:20066800

We mapped the HH212 Class 0 outflow in SiO(2--1, 5--4) and continuum using the PdBI in its extended configurations. The unprecedented angular resolution (down to 0.34") allows accurate comparison with a new, deep H2 image obtained at the VLT. The SiO emission is confined to a highly-collimated bipolar jet (width 0.35") along the outflow axis. The jet can be traced down to within 500 AU of the protostar, in a region that is heavily obscured in H2 images. Where both species are detected, SiO shows the same overall kinematics and structure as H2, indicating that both molecules are tracing the same material. We find that the high-velocity SiO gas near the protostar is not tracing a wide-angle wind but is already confined to a flow inside a narrow cone of half-opening angle < 6 deg.

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