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Star Formation Studies

Outflow detection in a 70 μm dark high-mass core
Image Credit: Siyi Feng
Outflow detection in a 70 μm dark high-mass core
A Compilation of the observations on G28.34 S, including dust emission observed by Herschel, ATLASGAL, SMA, NOEMA, and ALMA, and molecular line emissions of C18O and SiO observed by IRAM 30M, NOEMA, and ALMA. These images highlight the detection of a bipolar molecular outflow toward the dark high-mass core G28.34 S.
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