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Astrometry of 6.7 GHz Methanol Maser toward W 3(OH) with Japanese VLBI Network

TLDR
In this paper, the results of multiepoch VLBI observations for a 6.7 GHz methanol maser toward the UC H II region of W 3(OH) with Japanese VLBi Network (JVN) were derived, and the trigonometric annual parallax to be 0.598 ˙ 0.067 mas.
Abstract
We present the results of multiepoch VLBI observations for a 6.7 GHz methanol maser toward the UC H II region of W 3(OH) with Japanese VLBI Network (JVN). Based on phase-referencing VLBI astrometry, we derived the trigonometric annual parallax to be 0.598 ˙ 0.067 mas, corresponding to a distance of 1.67 +0:21 � 0:17 kpc. This is the first detection of parallax for a 6.7 GHz methanol maser with JVN, and demonstrates that JVN/VERA is capable of conducting VLBI astrometry for 6.7 GHz methanol maser sources within few kpc from the Sun. Based on in-beam mapping of the W 3(OH) methanol maser, we also measured the internal proper motions of its 6.7 GHz methanol maser for the first time. The internal proper motions basically show north–south expansion with a velocity of few km s � 1 , being similar to OH masers. The spatial distribution and the internal proper motions of 6.7 GHz

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Trigonometric parallaxes of star-forming regions in the Sagittarius spiral arm

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Microarcsecond Radio Astrometry

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The First VERA Astrometry Catalog

TL;DR: In this paper, the authors present the first catalog from the Japanese VLBI (Very Long Baseline Interferometer) project VERA (VLBI Exploration of Radio Astrometry).
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Capabilities and prospects of the East Asia Very Long Baseline Interferometry Network

TL;DR: The East Asia Very Long Baseline Interferometry Network (EAVN) consists of 21 radio telescopes whose equipment and frequency setup allow fine imaging of jets in active galaxies, high-accuracy astrometry of masers and pulsars, and spacecraft positioning as mentioned in this paper.
References
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Journal ArticleDOI

The distance to the Perseus spiral arm in the Milky Way.

TL;DR: The distance to the massive star–forming region W3OH in the Perseus spiral arm of the Milky Way is measured by triangulation, with Earth's orbit as one segment of a triangle, using the Very Long Baseline Array, resolving the long-standing problem that there is a discrepancy between different techniques used to determine distances.
Journal ArticleDOI

The distance to the center of the Galaxy - H2O maser proper motions in Sagittarius B2(N)

TL;DR: In this article, the proper motions of the maser spots are determined by applying the technique known as statistical parallax, and if organized motions are evident in the proper motion, one can model the source to estimate its the distance.
Journal ArticleDOI

Trigonometric parallaxes of 6.7 GHz methanol masers

TL;DR: In this paper, the 6.7 GHz methanol maser transition is used to perform high-precision astrometry to obtain accurate distances to the host regions of massive star-forming regions.
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