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

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.