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Water Maser Motions in W3(OH) and a Determination of Its Distance

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Hachisuka, K., Brunthaler, A., Menten, K. M., Reid, M. J., Imai, H., Hagiwara, Y., Miyoshi, M., Horiuchi, S., Sasao, T.·2006·The Astrophysical Journal

Abstract

We report phase-referencing VLBA observations of H 2 O masers near the star-forming region W3(OH) to measure their parallax and absolute proper motions. The measured annual parallax is 0.489 ± 0.017 mas (2.04 ± 0.07 kpc), where the error is dominated by a systematic atmospheric contribution. This distance is consistent with photometric distances from previous observations and with the distance determined from CH 3 OH maser astrometry presented in a related paper. We also find that the source driving the H 2 O outflow, the "TW-object," moves with a three-dimensional velocity of >7 km s -1 relative to the ultracompact H II region W3(OH).

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Metadata

Authors
Hachisuka, K., Brunthaler, A., Menten, K. M., Reid, M. J., Imai, H., Hagiwara, Y., Miyoshi, M., Horiuchi, S., & Sasao, T.
Venue
The Astrophysical Journal
Published
2006-07
Volume
645
Issue
1
Pages
337-344
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2046202567
Cited by
201
References
0
FWCI
10.61
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Water Maser Motions in W3(OH) and a Determination of Its Distance. https://app.cochat.ai/papers/10.1086/502962
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Hachisuka, K., Brunthaler, A., Menten, K. M., Reid, M. J., Imai, H., Hagiwara, Y., Miyoshi, M., Horiuchi, S., & Sasao, T. (2006). Water Maser Motions in W3(OH) and a Determination of Its Distance. The Astrophysical Journal. https://doi.org/10.1086/502962

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