Water Maser Emission Around Low/Intermediate Mass Evolved Stars
Konferensbidrag (offentliggjort, men ej förlagsutgivet), 2012

We present results of Very Long Baseline Array (VLBA) polarimetric 22 GHz H2O maser observations of a number of low/intermediate mass evolved stars. We observed 3 Miras (Ap Lyn, IK Tau and IRC+60370), 1 semi-regular variable (RT Vir) and 1 pPN (OH231.8+4.2). Circular polarization is detected in the H2O maser region of OH231.8+4.2 and we infer a magnetic field of |B||| = ~45 mG. This implies an extrapolated magnetic field of ~2.5 G on the surface of the central star. The preliminary results on RT Vir and IRC+60370 also indicate the first detection of weak H2O maser linear polarization.

stars: AGB and post-AGB



magnetic fields


M.L. Leal-Ferreira

Wouter Vlemmings

Chalmers, Rymd- och geovetenskap, Radioastronomi och astrofysik

P.J. Diamond

A Kemball

N. Amiri

J. F. Desmurs

Proceedings of the International Astronomical Union

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

Vol. 8 79 - 80


Astronomi, astrofysik och kosmologi


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