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

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arxiv 1103.3139 v1 pith:ZABZSFAA 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
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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.

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