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

Abstract

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

References in corpus (2)

• Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
• Search for Compact Extragalactic Radio Sources Near Massive Star Forming Regions

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