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arXiv · 0811.0704

Trigonometric Parallaxes of Massive Star Forming Regions: IV. G35.20-0.74 and G35.20-1.74

B. Zhang·X. W. Zheng·M. J. Reid·K. M. Menten·Y. Xu·L. Moscadelli·A. Brunthaler
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Abstract

We report trigonometric parallaxes for the high-mass star forming regions G35.20-0.74 and G35.20-1.74, corresponding to distances of 2.19 (+0.24 -0.20) kpc and 3.27 (+0.56 -0.42) kpc, respectively. The distances to both sources are close to their near kinematic distances and place them in the Carina-Sagittarius spiral arm. Combining the distances and proper motions with observed radial velocities gives the locations and full space motions of the star forming regions. Assuming a standard model of the Galaxy, G35.20-0.74 and G35.20-1.74 have peculiar motions of ~13 km/s and ~16 km/s counter to Galactic rotation and ~9 km/s toward the North Galactic Pole.

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B. Zhang, X. W. Zheng, M. J. Reid, K. M. Menten, Y. Xu, L. Moscadelli, A. Brunthaler. 2008-11-05. Trigonometric Parallaxes of Massive Star Forming Regions: IV. G35.20-0.74 and G35.20-1.74. https://doi.org/10.1088/0004-637x%2F693%2F1%2F419

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