Description of source "G 329.47+0.50" from McCarthy et el. (2018c)

The majority of class I maser emission is clustered around the 6.7-GHz maser in the centre of the field. This class II source is on the eastern edge of an EGO (classified as a likely outflow candidate by Cyganowski et al. (2008)). The majority of 95-GHz maser emission in this source is arranged in a line extending from the position of the 6.7-GHz maser towards the south-east.