SIMBAD references

Far red spectra for 22 stars in the Camelopardalis and the northern Perseus dark clouds, suspected to be pre-main-sequence objects (YSOs), are obtained. This evolutionary status is confirmed for ten stars located in the dust and molecular cloud close to the high-mass protostar GL490, four stars near the HII region Sh2-205 and one star in the dark cloud TGU1041. All of these objects exhibit emission in the Hα line and some of them emission in the OI and CaII lines. The spectral energy distributions, equivalent widths of the emission lines and approximate spectral classes are determined. Evolutionary stages of the stars are estimated from 2MASS J, H, K_s, IRAS and MSX infrared photometry. Now we have spectral confirmation of the YSO status for 14 stars in the GL490 area and 8 stars at Sh2-205. Their spectral types are from A to K, but most of them are either Herbig Ae stars or intermediate objects between T Tauri type and Herbig stars. Both these star forming regions are located near the outer edge of the Local arm at a distance of ∼900 pc.