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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).

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Dades d'Observació i Astrometria

Constel·lació:Gemini
Ascensió Recta:07h54m04.36s
Declinació:+29°12'41.0"
Magnitud Aparent:8.266
Distancia:10000000 parsecs
Moviment propi RA:35.1
Moviment propi Dec:-54.5
B-T magnitude:10.017
V-T magnitude:8.411

Catàlegs i designacions:
Noms Propis
HD 1989HD 64232
TYCHO-2 2000TYC 1937-329-1
USNO-A2.0USNO-A2 1125-05407080
HIPHIP 38586

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