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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.
| CCD astrometry and instrumental {DELTA}V photometry of wide visual double stars. IV. Differential measurements of northern pairs.
We present relative positions and instrumental visual magnitudedifferences ({DELTA}V) of 101 northern wide double star components. Themean accuracy of the magnitude differences is 0.01 magnitudes, of theangular separation 0.04 arcseconds, and of position angle 0.13 degrees.Most of the programme pairs are targets of the HIPPARCOS mission andthey have been often observed during the last 150 years.
| Photographic measures of double stars
Photographically determined individual relative positions are given for20 wide binaries over the period 1977-1981. Almost 60 percent of thesepositions are for the two systems 61 Cygni and 16 Cygni. Also given areweighted annual normal points.
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| Takýmyýldýz: | Zurafa |
| Sað Açýklýk: | 03h41m06.09s |
| Yükselim: | +60°39'23.7" |
| Görünürdeki Parlaklýk: | 9.506 |
| özdevim Sað Açýklýk: | 14.3 |
| özdevim Yükselim: | -16.2 |
| B-T magnitude: | 9.966 |
| V-T magnitude: | 9.544 |
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