FIRST BYURAKAN SPECTRAL SKY SURVEY. STARS OF LATE SPECTRAL TYPES.

A 10th list of late-type M and C stars found on plates of the First Byurakan Spectral Sky Survey in the -11° <- delta <-7° belt with an area of about 1070 deg^ is given. The list contains data on 169 red stars, 117 of which were found for the first time: 8 are new C stars, 3 are C-star candidates, 104 are M stars, I is either an M or an S star, and I object on the survey plate cannot be classified. Of the 1 17 objects, 47 are unidentified IRAS sources. A statistical analysis of the objects that are and are not identified with IRAS sources shows that the identified stars are, with a high probability, brighter and have relatively more massive envelopes. Two stars were found to have fairly large brightness variability (with an amplitude of at least 6ʹ".0). Gas-dust shells are assumed lo exist around nine of the IRAS sources. The equatorial coordinates, spectral types, and stellar magnitudes, determined on Palomar E maps, are given for the selected objects.