Bow shocks in water fountain jets
Paper in proceeding, 2017

We briefly introduce the VLBI maser astrometric analysis of IRAS 18043-2116 and IRAS 18113-2503, two remarkable and unusual water fountains with spectacular bipolar bow shocks in their high-speed collimated jet-driven outflows. The 22 GHz H2O maser structures and velocities clearly show that the jets are formed in very short-lived, episodic outbursts, which may indicate episodic accretion in an underlying binary system.

masers

techniques: Interferometric

stars: AGB and post-AGB

astrometry

Author

G. Orosz

Kagoshima University

Joint Institute for VLBI in Europe (JIVE)

J. F. Gomez

Institute of Astrophysics of Andalusia (IAA)

Daniel Tafoya

Chalmers, Earth and Space Sciences, Onsala Space Observatory

Galactic Astrophysics

H. Imai

Kagoshima University

J. M. Torrelles

Institute of Space Studies of Catalonia (IEEC)

Ann Njeri Ngendo

University of Nairobi

R. A. Burns

Joint Institute for VLBI in Europe (JIVE)

Kagoshima University

Proceedings of the International Astronomical Union

1743-9213 (ISSN) 1743-9221 (eISSN)

Vol. 13 S336 351-354

IAU Symposium No.336, 2017
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Subject Categories

Globalization Studies

Astronomy, Astrophysics and Cosmology

Oceanography, Hydrology, Water Resources

Infrastructure

Onsala Space Observatory

DOI

10.1017/S1743921317009589

More information

Latest update

4/1/2021 1