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A&A 393, L33-L36 (2002)
DOI: 10.1051/0004-6361:20021169
Letter
Astrometry of the stellar image of U Her amplified by the circumstellar 22 GHz water masers
W. H. T. Vlemmings1, H. J. van Langevelde2 and P. J. Diamond31 Sterrewacht Leiden, Postbus 9513, 2300 RA Leiden, The Netherlands
2 Joint Institute for VLBI in Europe, Postbus 2, 7990 AA Dwingeloo, The Netherlands
3 Jodrell Bank Observatory, University of Manchester, Macclesfield, Cheshire, SK11 9DL, England, UK
(Received 10 July 2002 / Accepted 9 August 2002 )
Abstract
The 22 GHz H
2O masers in the circumstellar envelope of
the Mira variable star U Her have been observed with MERLIN using a
phase referencing technique to determine accurate astrometric
positions. The positions were compared with the optical positions
obtained with the Hipparcos satellite to an accuracy of
18 mas. The
absolute radio position of the brightest H
2O maser spot is found to
match the optical position, indicating that this spot is the stellar
image amplified by the maser screen in front of it. The occurrence of
an amplified image in the 22 GHz maser can be used to accurately
determine the positions of the H
2O with respect to the star as well
as with respect to the SiO and OH masers. Our observations seem
to indicate that the star is not in the centre of the distribution of
maser spots, which has been interpreted as a ring.
Key words: masers -- stars: circumstellar matter -- stars: individual: U Her -- stars: AGB and post-AGB -- techniques: interferometric -- astrometry
Offprint request: W. H. T. Vlemmings, vlemming@strw.leidenuniv.nl
SIMBAD Objects
© ESO 2002
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