Description of source "17463-3128" from Slysh et al. (1999)

This IRAS source is also associated with OH maser of the Class Ib (emission only at 1667 GHz; Slysh et al. 1994b) at the velocity 9.4 km s1. The 6.7 GHz maser was also detected by van der Walt et al. (1995).

Spectra look similar, but the ux of the main feature at 5 km s1 is different: 31 Jy in our spectrum against 17 Jy according to van der Walt et al. (1995). This difference is a result of our higher velocity resolution and disappears when we compare our low-resolution spectrum with that of van der Walt et al. (1995).