Abstract
Some evolved stars in the pre-planetary nebula phase produce highly collimated molecular outflows that resemble the accretion-driven jets and outflows from pre-main-sequence stars. We show that IRAS 16342-3814 (the Water Fountain Nebula) is such an object and present K-band integral field spectroscopy revealing a fast (>150kms -1) bipolar H 2 outflow. The H2 emission is shock excited and may arise in fast-moving clumps, accelerated by the previously observed precessing jet. The total luminosity in H2 is 0.37 L ⊙, which is comparable with that of accretion-powered outflows from Class 0 protostars. We also detect CO overtone bandhead emission in the scattered continuum, indicating hot molecular gas close to the centre, a feature also observed in a number of protostars with active jets. It seems likely that the jet and outflow in IRAS 16342-3814 are powered by accretion on to a binary companion
| Original language | English |
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| Pages (from-to) | 346-355 |
| Journal | Monthly Notices of the Royal Astronomical Society (MNRAS) |
| Volume | 421 |
| Issue number | 1 |
| Early online date | 23 Jan 2012 |
| DOIs | |
| Publication status | Published - Mar 2012 |