W11449  = ADS8811C {delta}m=1.7, 8.3 arcsec), m_v_ from SIMBAD. 
W11450  = ADS8811AB {delta}m=1.4, 0.3 arcsec) has a composite spectrum. 
W11450  The primary correlation peak appears to be constant at a velocity of 
W11450   -0.26+/-0.11 from 137 exposures; the secondary peak is itself a 
W11450   single-lined spectroscopic binary. The gamma velocity for its orbital 
W11450   solution is -4.48+/-0.43; the system represented by the secondary peak 
W11450   probably has slightly more mass than the primary, so we estimate that 
W11450   the center of mass velocity should be about -2.4+/-0.5 for this triple 
W11450   system, (see also Mazeh and Latham 1988). 
W12096N G-band spectral type = Gl. 
W12965  spectral types from Latham et al. (1984ApJ...281L..41L).
W12966  spectral types from Latham et al. (1984ApJ...281L..41L). 
W13781  = ADS8826C {delta}m=3.0, 73.4 arcsec). 
W13784  = ADS8826AB {delta}m=4.0, 0.7 arcsec); only one correlation peak is 
W13784   seen for our spectra. 
W20942  visual companion {detla}m~5, 20 arcsec)
W21939  has a composite spectrum. The primary correlation peak appears to be 
W21939   constant at a velocity of -33.60+/-0.03 from 75 exposures; the 
W21939   secondary peak is itself a single-lined spectroscopic binary.  
W21939   The gamma velocity of its orbital solution is -36.03+/-0.42; 
W21939   the system represented by the secondary peak probably has slightly more
W21939   mass than the primary, so we estimate the center of mass velocity 
W21939   should be about -34.8+/-0.5 for this triple system. 
W25140  = ADS8788 {delta}m=4.5, 3.4 arcsec); g-band spectral type = F6. 
W31640  = ADS8731 {delta}m=9.3, 5.2 arcsec). 
W33427  G-band spectral type = F9. 
W33433  G-band spectral type = F5. 
W34059  the observed star at this position appears much fainter than V=12. 
W34584  weak CaII and MgII. Greenstein and Sargent (1974) 
W34584   assign a distance of 3532 pc. 
W40661  calcium, hydrogen, metal-line spectral types = A3, F2, F0 respectively.
W41083  = ADS8803 {delta}m=0.4, 4.0 arcsec). 
W41387  has a composite spectrum. The primary correlation peak appears to be 
W41387   constant at a velocity of -35.57+/-0.35 from 111 exposures; the 
W41387   secondary peak is itself a single-lined spectroscopic binary.  
W41387   The gamma velocity of its orbital solution is -35.36+/-0.19; 
W41387   the system represented by the secondary peak probably has slightly 
W41387   more mass than the primary, so we estimate the center of mass velocity
W41387   should be about -35.45+/-0.20 for this triple system. 
W42404  G-band spectral type = F3. 
W42574  Bond (private communication) reports that this star is a K giant, based
W42574   on Stroemgren photometry, and thus is unlikely to be at the same 
W42574   distance as W42576. 
W42576  calcium, hydrogen, metal-line spectral types = A4, Fl, F2 respectively. 
W44485  visual binary (12 arcsec). 
W44496  = ADS8827 {delta}m=0.5, 1.4 arcsec). 
W50462  = ADS8777 {delta}m=5.5, 6.3 arcsec). 
W51432  visual companion {delta}m=1.7, 17 arcsec). 
W52091  visual companion {delta}m~2, 18 arcsec). 
W60228  = ADS8748 {delta}m=3.0, 1.0 arcsec). 
W61473  calcium II emission
W61990  G-band spectral type = GO. 
W62717  G-band spectral type = F5. 
W64308  the position for this star may be in error.