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Based on new observations during 2015-2020 and published data, the unusualeruptive variables PV Cep and V350 Cep are examined. It is shown that PV Cepunderwent a regular outburst followed by a drop in brightness that lastedoverall from 2011 to 2019 and is still in a deep minimum. The outburst wasaccompanied by substantial changes in the intensity and profiles of a number oflines, including Ha, [SII], and [OI]. The forbidden lines generally havenegative radial velocities and can be divided into four components, withvariable velocities and relative intensities. V350 Cep essentially is at amaximum brightness level over the entire time and its spectrum is practicallyunaltered. The available data suggest that the pronounced P Cyg profile of theHa line in the spectrum of V350 Cep appeared several years after the luminosityrise, in 1986. The luminosities of the stars in the current state are estimatedto be 20 L(sun) and 3.3 L(sun), respectively. It is concluded that both starsmay represent a so-called intermediate objects between the FUor and EXorclasses.

PV Cep and V350 Cep: stars on the way between FUors AND EXors