Description of source "20056+3350" from Gomez-Ruiz et al. (2016)

Although M98 did not detect radio continuum emission in this field, Jenness et al. (1995) report weak (0.6–0.9 mJy) 8 GHz emission located about 2″ from the maser positions.

Although this continuum emission—located so close to the maser positions—is interesting, we do not count Mol 115 as a source with a UC H II region, because the quite low flux density suggests that the origin of the emission is not photoionization by a young, early-type star, but rather is due to some other mechanism (e.g., Rodríguez et al. 2012).