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Speckle Interferometry at the US Naval Observatory. VIII.
The results of 2044 speckle interferometric observations of doublestars, made with the 26 inch (66 cm) refractor of the US NavalObservatory, are presented. Each speckle interferometric observation ofa system represents a combination of over a thousand short-exposureimages. These observations are averaged into 1399 mean positions andrange in separation from 0.16" to 14.97", with a mean separation of2.51". This is the eighth in a series of papers presenting measuresobtained with this system and covers the period 2001 March 18 through2001 December 30.
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We publish 1879 radial velocities of stars distributed in 105 fields of4^{\circ} \times 4^{\circ}. We continue the PPO series \cite[(Fehrenbachet al. 1987;]{Feh87} \cite[Duflot et al. 1990, 1992 and 1995),]{Du90}using the Fehrenbach objective prism method. Table 1 only available inelectronic form at CDS via to cdsarc.u-strasbg.fr (130.79.128.5) or viahttp://cdsweb.u-strasbg.fr/Abstract.html
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Datos observacionales y astrométricos
| Constelación: | Osa Mayor |
| Ascensión Recta: | 08h59m00.62s |
| Declinación: | +63°25'42.8" |
| Magnitud Aparente: | 7.243 |
| Distancia: | 200.803 parsecs |
| Movimiento Propio en Ascensión Recta: | -17.4 |
| Movimiento Propio en Declinación: | -34 |
| B-T magnitude: | 8.537 |
| V-T magnitude: | 7.35 |
Catálogos y designaciones:
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