ALS 11633   spectral binaries
ALS 17620   visual binaries
ALS 17622   visual binaries
SMV89-159   spectral binaries
SMV89-185   visual binaries
SMV89-188   spectral binaries
SMV89-248   = V2200 Cyg (B9p, alpha^2^ CVn type)
VI Cyg 5    = V729 Cyg, EB
LS02-40     IS (interstellar band at 443nm) band slight
LS02-209    IS (interstellar band at 443nm) band moderate, AV=2.9
LS02-217    IS (interstellar band at 443nm) band slight, He slightly strong,
LS02-217     AV=2.3
LS02-222    very strong IS (interstellar band at 443nm) band,
LS02-222     quite strong IS Ca K, AV=4.2
LS02-229    sharp hydrogen line cores, moderate IS (interstellar band at 443nm)
LS02-229     band, Hg-Mn, Cr-Sr
LS02-230    emission in H and He, with normal decrement, spectral class is an
LS02-230     estimate from H wings and He I D-series,
LS02-230     IS (interstellar band at 443nm) band moderate, AV=2.5
LS02-267    IS (interstellar band at 443nm) band strong, AV=2.2
LS02-401    IS (interstellar band at 443nm) band slight,
LS02-401     IS Ca K quite strong, AV=1.9
LS02-463    all He lines are filled in by emission, AV=1.9
LS02-476    IS (interstellar band at 443nm) band moderate; AV=2.7
LS02-537    IS (interstellar band at 443nm) band moderate, AV=2.2
LS02-584    IS (interstellar band at 443nm) band moderate,
LS02-584     IS Ca K line strong, AV=3.9
LS02-608    Balmer line decrement weak, IS (interstellar band at 443nm) band
LS02-608     slight, IS Ca K line moderate, AV=1.8
LS02-691    noisy spectrum, IS (interstellar band at 443nm) band strong, 
LS02-691     AV=5.2.