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arxiv 1407.1609 v1 pith:LWEQEQM6 submitted 2014-07-07 astro-ph.GA

Trigonometric Parallaxes of Star Forming Regions in the Perseus Spiral Arm

classification astro-ph.GA
keywords galacticperseusspiralformingmotionsparallaxesregionsstar
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We report trigonometric parallaxes and proper motions of water masers for 12 massive star forming regions in the Perseus spiral arm of the Milky Way as part of the Bar and Spiral Structure Legacy (BeSSeL) Survey. Combining our results with 14 parallax measurements in the literature, we estimate a pitch angle of 9.9 +/- 1.5 degrees for a section of the Perseus arm. The three-dimensional Galactic peculiar motions of these sources indicate that on average they are moving toward the Galactic center and slower than the Galactic rotation.

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Cited by 1 Pith paper

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  1. Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors

    astro-ph.GA 2026-07 conditional novelty 4.0

    A Gaia DR3-based census of 105,971 OB stars within 2 kpc maps local Galactic structure and identifies over 4,200 core-collapse supernova or black hole progenitor candidates.