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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).
| Speckle Interferometry of New and Problem Hipparcos Binaries. II. Observations Obtained in 1998-1999 from McDonald Observatory
The Hipparcos satellite made measurements of over 9734 known doublestars, 3406 new double stars, and 11,687 unresolved but possible doublestars. The high angular resolution afforded by speckle interferometrymakes it an efficient means to confirm these systems from the ground,which were first discovered from space. Because of its coverage of adifferent region of angular separation-magnitude difference(ρ-Δm) space, speckle interferometry also holds promise toascertain the duplicity of the unresolved Hipparcos ``problem'' stars.Presented are observations of 116 new Hipparcos double stars and 469Hipparcos ``problem stars,'' as well as 238 measures of other doublestars and 246 other high-quality nondetections. Included in these areobservations of double stars listed in the Tycho-2 Catalogue andpossible grid stars for the Space Interferometry Mission.
| Photometry of long-period Algol binaries. VI - Multicolor photometric solutions for RZ CANCRI
New intermediate-band photometry of the late-giant eclipsing system RZCNc is used to obtain photometric solutions, both with the Popper (1976)spectroscopic mass ratio and by allowing the mass ratio andgravity-darkening coefficients to vary. New y observations are combinedwith earlier V data of Lenouvel (1957) and Broglia and Conconi (1973) inone solution set. Additional solutions are obtained from the newobservations. The mean photometric mass ratio is somewhat larger thanPopper's spectroscopic values; the general indeterminacy of photometricsolutions may explain this apparent discrepancy. Possible photometriceffects of a mass-transferring stream are discussed, and it is concludedthat such effects cannot account for the mass-ratio discrepancy.
| Photoelectric observations of RZ Cnc.
Abstract image available at:http://adsabs.harvard.edu/cgi-bin/nph-bib_query?1957AJ.....62..159L&db_key=AST
| Observations photoélectriques
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Pozíciós és asztrometriai adatok
| Csillagkép: | Rák |
| Rektaszcenzió: | 08h38m39.46s |
| Deklináció: | +31°09'38.3" |
| Vizuális fényesség: | 8.514 |
| Távolság: | 10000000 parszek |
| RA sajátmozgás: | -26.3 |
| Dec sajátmozgás: | -39.6 |
| B-T magnitude: | 10.126 |
| V-T magnitude: | 8.648 |
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