, Robert Lucas
, Stephane Guilloteau
Observatoire de Bordeaux, 33270 Floirac, France
IRAM, 300, rue de la Piscine, Domaine Universitaire,
38406 Saint-Martin-d'Hères, France.
to
in general. The optical and radio centers coincide within the uncertainties.
However, in the complex supergiants VY CMa and VX Sgr there is a clear offset
between the optical and radio positions. Spatial structure is present in our
SiO data since we have observed in several stars relative position offsets
larger than about 20-50 milliarcsec.
The radio and optical J2000 positions are compared and discussed, and we suggest that accurate position measurements of maser sources associated with stars may valuably contribute to the alignment of the fundamental optical and extragalactic reference frames.