Astrometry of W49N - OH43.8-0.1 H2O maser pair with VERA

dc.creatorHonma, Mareki
dc.date2004-12-30
dc.date.accessioned2026-07-25T12:21:30Z
dc.descriptionWe present the results of multi-epoch VERA observations of W49N - OH43.8-0.1 water maser pair. Based on the dual-beam VLBI observation with VERA, we successfully obtained the phase-referenced maps of OH43.8-0.1 with respect to the W49N reference spot for 3 epochs with a time span of 6 months. The maps were in good agreement with previous studies obtained with a single-beam VLBI, and were also consistent with each other with an accuracy of about 0.2 mas. Moreover, there are systematic, rather linear displacements of maser feature positions, which may be the relative proper motions of maser features caused by the Galactic rotation as well as internal motions of individual maser features.
dc.description2 pages. 1 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 201-202. Needs evn2004.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0412681
dc.identifierhttp://arxiv.org/abs/astro-ph/0412681
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/9678
dc.subjectAstrophysics
dc.titleAstrometry of W49N - OH43.8-0.1 H2O maser pair with VERA
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