Description of source "G30.79+0.20" from Ellingsen (2007)

this source was discovered by Caswell et al. (1995b) who found it to exhibit emission in two groups over a velocity range of 7589 km s1, similar to that observed by Szymczak et al. (2002). Fig. 6 shows emission over this range, but also a number of weak features near 100 km s1. Given that emission in this range was not observed on previous occasions, it is probably the nearby source G30.89+0.17 detected in the telescope sidelobes. The peak ux density of the emission near 76 km s1 has more than tripled in the period between 1992 and 2005.