Year: 2016
Type: article
Abstract: Aims. Previous observations of the young massive star formation region IRAS 19410+2336 have revealed strong outflow activity with several interacting outflows. We aim to get a better understanding of the outflow activity in this region by observing the SiO and H13CO+ emission with high angular resolution. SiO is known to trace shocked gas, which is often associated with young energetic outflows. With the H13CO+ data, we intend to better understand the distribution of the quiescent gaseous component of the region.
Source: Astronomy and Astrophysics
Authors: F. Widmann, H. Beuther, P. Schilke, T. Stanke
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W4297676507