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

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

2011-03-16

arxiv.org/abs/1103.3139v1

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

Scientific paper

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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