Description of source "G22.357+0.066" from Bartkiewicz et al. (2009)


The ATCA observations detected three maser spots (Walsh et al. 1998), while the EVN revealed 31 spots in 10 clusters. The strongest emission detected with both interferometers, at 80.0 km s−1, coincides to within 1.7". We de-tected new emission at close to 88.5 km s−1, 0.20–0.27" north of the brightest spot, but a 77.0 km s−1 spot reported by Walsh et al. (1998) was not redetected.