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In the first three papers of this series, about 200 objects in Camelopardalisand the nearby areas of Cassiopeia, Perseus and Auriga were suspected of beingpre-main-sequence stars in different stages of evolution. To confirm theevolutionary status of the 15 brightest objects, their far-red range (600--950nm) spectra were obtained. Almost all these objects are young stars withemissions in H alpha, OI, CaII and P9 lines. The equivalent widths of emissionlines and approximate spectral classes of the objects are determined.

Young Stars in the Camelopardalis Dust and Molecular Clouds. IV. Spectral Observations of the Suspected YSOs