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Far red spectra for 34 stars with V magnitudes between 15 and 18 in thedirection of the North America and Pelican nebulae (NAP) star-forming regionare obtained. Some of these stars were known earlier as emission-line objects,others were suspected as pre-main-sequence stars from photometry in the J, H,Ks and Vilnius systems. We confirm the presence of the H alpha line emission inthe spectra of 19 stars, some of them exhibit also emission in the O I and CaII lines. In some of the stars the H alpha absorption line is filled withemission. To estimate their evolutionary status, the spectral energydistributions, based on Vilnius, 2MASS, MSX and Spitzer photometry, areapplied. Only eight emission-line stars are found to be located at a distanceof the NAP complex. Others are either chromospherically active stars in frontof the complex or distant luminous stars with H alpha absorption and emissioncomponents. For five stars with faint emission the data are not sufficient toestimate their distance. One star is found to be a heavily reddenedK-supergiant located in the Outer arm. The stars, for which we failed toconfirm the emission in H alpha, are mostly red dwarfs located in front of theNAP complex, two of them could be binaries with L-type components. Taking intoaccount the stars suspected to be YSOs by their 2MASS colors we conclude thatthe NAP complex can possess a considerable population of young stars hiddenbehind the dust cloud.

Spectral analysis of YSOs and other emission-line stars in the North America and Pelican nebulae region