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Sottometti un nuovo articolo| CCD astrometry and components instrumental magnitude difference of 432 Hipparcos wide visual double stars Context: We measured the angular separations, position angles, ΔV, Δ y and Δ I of wide visual double stars during the period2003-2005. At least one component of the double stars in our sample hasan entry in the Hipparcos catalogue.  Aims: Our measurements are acontribution to the study of the nature of these double stars.  Methods: The northern double stars of the project were observed with the1.2 m telescope of the Kryonerion observatory and the southern with the1.0 m SAAO. We performed multiple-exposure CCD imaging of our targetsand used the standard procedure of data reduction and astrometric CCDcalibrations.   Results: We present measurements of 213 northern and 219southern wide binaries.Based on observations made at Kryonerion Observatory of the NationalObservatory of Athens, Greece, and the South African AstronomicalObservatory. Full Table 1 and Tables 2, 3 are only available inelectronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr(130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/472/1055
 
 
 |  | Photovisual Magnitude Differences for 169 Double Stars Photovisual magnitude differences determined from multi-exposurephotographic plates for 169 double stars are presented. The separationsrange from 1.5'' to 113\arcsec, and the photovisual magnitudedifferences vary from 0.03 to 6.14 magnitudes. The internal mean errorof a single magnitude difference estimate is +/-0.064 magnitude.
 
 
 |  | A second list of wide visual binaries Not Available
 
 
 |  | A second list of wide visual binaries Not Available
 
 
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 Osservazione e dati astrometrici
| Costellazione: | Orsa Minore |  | Ascensione retta: | 16h40m57.37s |  | Declinazione: | +82°21'53.1" |  | Magnitudine apparente: | 8.907 |  | Distanza: | 293.255 parsec |  | Moto proprio RA: | -18.4 |  | Moto proprio Dec: | 10.4 |  | B-T magnitude: | 10.042 |  | V-T magnitude: | 9.001 |  Cataloghi e designazioni:
 
 
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