Abstract
We present the first internal motion measurement of the 6.7-GHz methanol maser within S269, a small HII region in the outer Galaxy, which was carried out in 2006 and 2011 using the Japanese VLBI Network (JVN). Several maser groups and weak isolated spots were detected in an area spanning ̃200 mas (1000AU). Three remarkable maser groups are aligned at a position angle of 80°. Two of three maser groups were also detected by a previous observation in 1998, which allowed us to study a long-term position variation of maser spots from 1998 to 2011. The angular separation between the two groups increased by ̃10 mas, which corresponds to an expansion velocity of ̃10 km s -1. Some velocity gradient (̃10-2 km s-1 mas-1) in the overall distribution was found. The internal motion between the maser groups support the hypothesis that the methanol masers in S269 could trace a bipolar outflow. © 2013. Astronomical Society of Japan.
Author supplied keywords
Cite
CITATION STYLE
Sawada-Satoh, S., Fujisawa, K., Sugiyama, K., Wajima, K., & Honma, M. (2013). Internal motion of 6.7-GHz methanol masers in HII region S269. Publications of the Astronomical Society of Japan, 65(4). https://doi.org/10.1093/pasj/65.4.79
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.