Prof. Tachibana issued a press release
ALMA image showing AlO around the star at wavelengths of 497 gigahertz(left) and 650 gigahertz (right). Image: © 2019 Astrophysical Journal Letters/Shogo Tachibana
Spatial distribution of AlO in a high mass protostar candidate Orion Source I
This research results appear in Astrophysical Journal Letters.
doi.org/10.3847/2041-8213/ab1653
