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Radial velocity measurements. IV - Ground-based accompaniment to the HIPPARCOS observation program The paper presents 396 radial velocities of stars distributed in 19fields of 4 x 4 degrees. The study employs the Fehrenbach objectiveprism method and the same measuring technique used in a previous paper(Fehrenbach et al., 1987).
 
  |  Miscellaneous spectroscopic notes Results of slit-spectrograph observations are reported for approximately260 stars. The data presented range from recognition of many new Ap, Am,and other unusual stars to H-alpha observations of early-typesupergiants and Be stars. The material discussed was obtained over thepast 40 years at a number of U.S. observatories and at the DominionAstrophysical Observatory in Victoria, B.C.
 
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Observation and Astrometry data
| Constellation: | Ursa Major |  
    | Right ascension: | 09h27m01.39s |  
    | Declination: | +47°46'23.6" |  
    | Apparent magnitude: | 7.564 |  
    
        | Distance: | 105.82 parsecs |  
        
    
    | Proper motion RA: | -2.1 |  
    | Proper motion Dec: | 3.1 |  
    | B-T magnitude: | 7.906 |  
    | V-T magnitude: | 7.593 |  
    
 
 
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