Trigonometric Parallaxes of Massive Star Forming Regions: VIII. G12.89+0.49, G15.03-0.68 (M17) and G27.36-0.16

A. Brunthaler; B. Zhang; K. M. Menten; L. Moscadelli; M. J. Reid; X. W. Zheng; Y. Xu

arxiv: 1103.3139 · v1 · pith:ZABZSFAAnew · submitted 2011-03-16 · 🌌 astro-ph.GA · astro-ph.SR

Trigonometric Parallaxes of Massive Star Forming Regions: VIII. G12.89+0.49, G15.03-0.68 (M17) and G27.36-0.16

Y. Xu , L. Moscadelli , M. J. Reid , K. M. Menten , B. Zhang , X. W. Zheng , A. Brunthaler This is my paper

classification 🌌 astro-ph.GA astro-ph.SR

keywords formingmassiveparallaxesregionsstartrigonometriccarina-sagittariuscorresponding

0 comments

read the original abstract

We report trigonometric parallaxes for three massive star forming regions, corresponding to distances of $2.34^{+0.13}_{-0.11}$ kpc for G12.89+0.49 (also known as IRAS 18089-1732),$1.98^{+0.14}_{-0.12}$ kpc for G15.03-0.68 (in the M17 region), and $8.0^{+4.0}_{-2.0}$ kpc for G27.36-0.16. Both G12.89+0.49 and G15.03-0.68 are located in the Carina-Sagittarius spiral arm.

This paper has not been read by Pith yet.

discussion (0)

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW
astro-ph.GA 2026-05 unverdicted novelty 5.0

High-resolution magnetic field maps of M17 SW reveal gravity-dominated energy budget with magnetic fields regulating collapse and accretion channels in a near-equipartition state.