arXiv:1103.3139 [astro-ph.GA]AbstractReferencesReviewsResources
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
Published 2011-03-16Version 1
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.
Categories: astro-ph.GA, astro-ph.SR
Keywords: massive star forming regions, report trigonometric parallaxes, carina-sagittarius spiral arm, m17 region
Tags: journal article
Related articles: Most relevant | Search more
arXiv:1304.2041 [astro-ph.GA] (Published 2013-04-07)
Trigonometric Parallaxes of Massive Star Forming Regions: G012.88+0.48 and W33
arXiv:1004.3290 [astro-ph.GA] (Published 2010-04-19)
Massive Star Forming Regions in the Galaxy using the Spitzer GLIMPSE Survey
arXiv:1803.03501 [astro-ph.GA] (Published 2018-03-09)
Infall and Outflow Motions towards a Sample of Massive Star Forming Regions from the RMS Survey