A fast bipolar H2 outflow from IRAS 16342-3814: An old star reliving its youth

T. Gledhill, K.P. Forde

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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 languageEnglish
Pages (from-to)346-355
JournalMonthly Notices of the Royal Astronomical Society
Volume421
Issue number1
Early online date23 Jan 2012
DOIs
Publication statusPublished - Mar 2012

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