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Cited article:

Rapidly evolving episodic outflow in IRAS 18113−2503: clues to the ejection mechanism of the fastest water fountain

G Orosz, J F Gómez, H Imai, D Tafoya, J M Torrelles, R A Burns, P Frau, M A Guerrero, L F Miranda, M A Perez-Torres, G Ramos-Larios, J R Rizzo, O Suárez and L Uscanga
Monthly Notices of the Royal Astronomical Society: Letters 482 (1) L40 (2019)
https://doi.org/10.1093/mnrasl/sly177

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

A. I. Gómez-Ruiz, L. Guzman-Ramirez, E. O. Serrano, D. Sánchez-Argüelles, A. Luna, F. P. Schloerb, G. Narayanan, M. S. Yun, R. Sahai, A. A. Zijlstra, M. Chavez-Dagostino, A. Montaña, D. H. Hughes and M. Rodríguez
Monthly Notices of the Royal Astronomical Society: Letters 467 (1) L61 (2017)
https://doi.org/10.1093/mnrasl/slw259

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

R. Sahai, W. H. T. Vlemmings, T. Gledhill, C. Sánchez Contreras, E. Lagadec, L-Å Nyman and G. Quintana-Lacaci
The Astrophysical Journal Letters 835 (1) L13 (2017)
https://doi.org/10.3847/2041-8213/835/1/L13

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

J. H. He, R. Szczerba, T. I. Hasegawa and M. R. Schmidt
The Astrophysical Journal Supplement Series 210 (2) 26 (2014)
https://doi.org/10.1088/0067-0049/210/2/26

From the ashes: JVLA observations of water fountain nebula candidates show the rebirth of IRAS 18455+0448

W. H. T. Vlemmings, N. Amiri, H. J. van Langevelde and D. Tafoya
Astronomy & Astrophysics 569 A92 (2014)
https://doi.org/10.1051/0004-6361/201423754

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

Jun-ichi Nakashima, Nico Koning, Nikolaus H. Volgenau, et al.
The Astrophysical Journal 759 (1) 61 (2012)
https://doi.org/10.1088/0004-637X/759/1/61

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

L. Cerrigone, K. M. Menten and T. Kamiński
Astronomy & Astrophysics 542 A15 (2012)
https://doi.org/10.1051/0004-6361/201118683

Extremely Strong 13CO J = 3→2 Line in the ``Water Fountain'' IRAS 16342−3814: Evidence for the Hot-Bottom Burning

Hiroshi Imai, Sze Ning Chong, Jin-Hua He, Jun-Ichi Nakashima, Chih-Hao Hsia, Takeshi Sakai, Shuji Deguchi and Nico Koning
Publications of the Astronomical Society of Japan 64 (5) (2012)
https://doi.org/10.1093/pasj/64.5.98

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
Proceedings of the International Astronomical Union 7 (S283) 484 (2011)
https://doi.org/10.1017/S1743921312012045

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

Bosco H. K. Yung, Jun-ichi Nakashima, Hiroshi Imai, et al.
The Astrophysical Journal 741 (2) 94 (2011)
https://doi.org/10.1088/0004-637X/741/2/94

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

Hiroshi Imai, Jin-Hua He, Jun-ichi Nakashima, Nobuharu Ukita, Shuji Deguchi and Nico Koning
Publications of the Astronomical Society of Japan 61 (6) 1365 (2009)
https://doi.org/10.1093/pasj/61.6.1365