Description of source "G 332.60-0.16" from McCarthy et el. (2018c)

There are two sites of class I methanol emission within this source. The 6.7-GHz maser is associated with the southern class I emission and a faint EGO (classified as likely outflow by Cyganowski et al. (2008)). Both 95-GHz maser components are situated on the western edge of this EGO, nearby (within 2 arc-sec) to the class II maser.