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Statistical Constraints for Astrometric Binaries with Nonlinear Motion
Useful constraints on the orbits and mass ratios of astrometric binariesin the Hipparcos catalog are derived from the measured proper motiondifferences of Hipparcos and Tycho-2 (Δμ), accelerations ofproper motions (μ˙), and second derivatives of proper motions(μ̈). It is shown how, in some cases, statistical bounds can beestimated for the masses of the secondary components. Two catalogs ofastrometric binaries are generated, one of binaries with significantproper motion differences and the other of binaries with significantaccelerations of their proper motions. Mathematical relations betweenthe astrometric observables Δμ, μ˙, and μ̈ andthe orbital elements are derived in the appendices. We find a remarkabledifference between the distribution of spectral types of stars withlarge accelerations but small proper motion differences and that ofstars with large proper motion differences but insignificantaccelerations. The spectral type distribution for the former sample ofbinaries is the same as the general distribution of all stars in theHipparcos catalog, whereas the latter sample is clearly dominated bysolar-type stars, with an obvious dearth of blue stars. We point outthat the latter set includes mostly binaries with long periods (longerthan about 6 yr).
| UV survey of certain fields of the sky with the Glazar space telescope
The Glazar telescope, installed on the Kvant module of the Mir spacestation, started regular observations in August 1987. This paperpresents results of the photometry of 15 stars detected by the Glazartelescope at 1640 A in an area of about 28 sq deg at high Galacticlongitudes.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Zincirli Prenses |
| Sað Açýklýk: | 00h10m48.49s |
| Yükselim: | +30°41'08.3" |
| Görünürdeki Parlaklýk: | 7.896 |
| Uzaklýk: | 250 parsek |
| özdevim Sað Açýklýk: | 0.5 |
| özdevim Yükselim: | -11.9 |
| B-T magnitude: | 7.931 |
| V-T magnitude: | 7.899 |
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