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TRIGONOMETRIC PARALLAXES OF MASSIVE STAR-FORMING REGIONS. I. S 252 & G232.6+1.0

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Reid, M. J., Menten, K. M., Brunthaler, A., Zheng, X. W., Moscadelli, L., Xu, Y.·2009·The Astrophysical Journal

Abstract

We are conducting a large program with the NRAO Very Long Baseline Array (VLBA) to measure trigonometric parallaxes of massive star-forming regions across the Milky Way. Here we report measurement of the parallax and proper motion of methanol masers in S 252 and G232.6+1.0. The parallax of S 252 is 0.476 ± 0.006 mas (2.10 +0.027 −0.026 kpc), placing it in the Perseus spiral arm. The parallax of G232.6+1.0 is 0.596 ± 0.035 mas (1.68 +0.11 −0.09 kpc), placing it between the Carina–Sagittarius and Perseus arms, possibly in a Local (Orion) spur of the Carina–Sagittarius arm. For both sources, kinematic distances are significantly greater than their parallax distances. Our parallaxes and proper motions yield full space motions accurate to ≈1 km s −1 . Both sources orbit the Galaxy ∼13 km s −1 slower than circular rotation.

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Metadata

Authors
Reid, M. J., Menten, K. M., Brunthaler, A., Zheng, X. W., Moscadelli, L., & Xu, Y.
Venue
The Astrophysical Journal
Published
2009-03-01
Volume
693
Issue
1
Pages
397-405
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2050740676
Cited by
181
References
0
FWCI
8.91
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: TRIGONOMETRIC PARALLAXES OF MASSIVE STAR-FORMING REGIONS. I. S 252 & G232.6+1.0. https://app.cochat.ai/papers/10.1088/0004-637x/693/1/397
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Reid, M. J., Menten, K. M., Brunthaler, A., Zheng, X. W., Moscadelli, L., & Xu, Y. (2009). TRIGONOMETRIC PARALLAXES OF MASSIVE STAR-FORMING REGIONS. I. S 252 & G232.6+1.0. The Astrophysical Journal. https://doi.org/10.1088/0004-637x/693/1/397

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