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Intermediate-Brightness Equatorial Spectrophotometric Standards We have obtained spectral energy distributions for 41 7m 8m stars nearthe celestial equator (δ=±3°). The λλ31007600 Å spectral range is studied with a spectral resolution of 50Å. The relative rms error in the visible is 1 2%, increasing to 35% towards the edges of the wavelength interval studied. All stars arereferenced to a single standard, the circumpolar star HD 221525. Thesynthetic colors of common stars are compared with those observed infour photometric systems: U BV, W BV R, uvby, and that of the TYCHOcatalog. The program stars are recommended as secondaryspectrophotometric standards.
 
  |  Optical observations of ultraviolet objects. I - Spectral classification of 103 stars /l = 200-275 deg/ Results are presented of a program of spectral classification of 103stars originally selected as ultraviolet objects from TD-1 satellitephotometry with the S2/68 experiment. Most of the objects appear to bespectroscopically normal stars; the method of selection yielded a sampleof relatively unreddened B stars at distances up to about 2 kpc. Thisresult is compared with recent studies of the spatial distribution ofinterstellar extinction in the same regions of the sky.
 
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תצפית ומידע אסטרומטרי
| קבוצת-כוכבים: | חד קרן |  
    | התרוממות ימנית: | 06h37m39.96s |  
    | סירוב: | +01°48'41.3" |  
    | גודל גלוי: | 7.782 |  
    
        | מרחק: | 374.532 פארסק |  
        
    
    | תנועה נכונה: | 0.7 |  
    | תנועה נכונה: | -8.1 |  
    | B-T magnitude: | 7.669 |  
    | V-T magnitude: | 7.773 |  
    
 
 
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