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• W2019440916 startingPage "1345" @default.
• W2019440916 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" @default.
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• W2019440916 date "2011-12-25" @default.
• W2019440916 modified "2023-10-12" @default.
• W2019440916 title "Astrometry of 6.7 GHz Methanol Maser toward W 3(OH) with Japanese VLBI Network" @default.
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• W2019440916 doi "https://doi.org/10.1093/pasj/63.6.1345" @default.
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