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Cited article:

First detection of CO lines in a water fountain star

J. H. He, H. Imai, T. I. Hasegawa, S. W. Campbell, J. Nakashima

A&A, 488 2 (2008) L21-L24

Published online: 2008-07-23

DOI: https://doi.org/10.1051/0004-6361:200810303

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Early science with the Large Millimeter Telescope: molecules in the extreme outflow of a protoplanetary nebula

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ALMA Observations of the Water Fountain Pre-planetary Nebula IRAS 16342-3814: High-velocity Bipolar Jets and an Expanding Torus

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OBSERVED RELATIONSHIP BETWEEN CO 2-1 AND DUST EMISSION DURING THE POST-ASYMPTOTIC-GIANT-BRANCH PHASE

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Sensitive CO and13CO survey of water fountain stars

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Extremely Strong13COJ= 3→2 Line in the ``Water Fountain'' IRAS 16342−3814: Evidence for the Hot-Bottom Burning

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CO STRUCTURE OF THE 21 μm SOURCE IRAS 22272+5435: A SIGN OF A JET LAUNCH?

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CO observations of water-maser post-asymptotic giant branch stars and detection of a high-velocity outflow in IRAS 15452–5459

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A fast bipolar H2 outflow from IRAS 16342−3814: an old star reliving its youth

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HIGH VELOCITY PRECESSING JETS FROM THE WATER FOUNTAIN IRAS 18286–0959 REVEALED BY VERY LONG BASELINE ARRAY OBSERVATIONS

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A complete survey of mm line emission from CO and 13CO in water fountain stars

J. Ricardo Rizzo, José F. Gómez, Luis F. Miranda, Mayra Osorio and Olga Suárez
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870 μm observations of evolved stars with LABOCA

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CO J = 3–2 Emission from the “Water Fountain” Sources IRAS 16342-3814 and IRAS 18286-0959

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