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Speckle observations with PISCO in Merate - II. Astrometric measurements of visual binaries in 2004
We present relative astrometric measurements of visual binaries takenduring the second semester of 2004 with the Pupil Interferometry Specklecamera and Coronagraph (PISCO) at the 1-m Zeiss telescope of the BreraAstronomical Observatory, in Merate, Italy. We performed 207 newobservations of 194 objects with angular separations in the range0.1-4.0 arcsec and an accuracy better than ~0.01 arcsec. Our samplecontains orbital couples as well as binaries whose motion is stilluncertain. Our purpose is to improve the accuracy of the orbits andconstrain the masses of the components.Those measurements show that the orbit of ADS 15115 needs to be revised;we propose a new orbit for this object.
| A preliminary compilation of DS-programme star positions
A catalog is presented of the double-star-program (DS-program) starpositions, listing right ascensions for 930 DSs and declinations for1225 DSs of the program. The positions were compiled from the observedvalues obtained between 1980 and 1987 with the meridian circles of sixUSSR observatories (the Moscow, Kazan', Kiev, Khar'kov, Odessa, andTashkent Observatories) and the Belgrade Observatory. The measurementsand the treatment of the observational material were performed using therelative method, and the FK-4 system stars were used as reference stars.
| Confirmation among visual multiples of an increase of AP stars with age
Open clusters with ages below certain threshold values contain no Apstars and those with greater ages contain numbers of Ap stars thatapparently increase with age. But in view of the few young clustersstudied, the data could also be interpreted in terms of randomdifferences in the frequencies of Ap stars between individual clusters,rather than an age effect. Data on 77 field visual multiple systems(that originated from many different clusters and associations) in whichthe primaries are O5-A1 stars and the secondaries occur in the absolutemagnitude range of the Ap stars were, therefore, obtained. Againspectral classification shows no Ap stars in systems with ages notgreater than 1,000,000 yr and a steady increase in Ap stars thereafter.The numerical agreement with the cluster data is good, confirming thatthe cluster data are exhibiting a real age effect.
| Micrometer measures of doubles stars. III.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1963AJ.....68...57V&db_key=AST
| Measures of double stars
Not Available
| Mesures micrométriques d'Etoiles Doubles
Not Available
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Группы:
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Наблюдательные данные и астрометрия
| Созвездие: | Цефей |
| Прямое восхождение: | 22h49m36.21s |
| Склонение: | +66°33'13.8" |
| Видимая звёздная величина: | 7.255 |
| Расстояние: | 248.139 парсек |
| Собственное движение RA: | 6 |
| Собственное движение Dec: | -10.5 |
| B-T magnitude: | 7.296 |
| V-T magnitude: | 7.259 |
Каталоги и обозначения:
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