Astrometric Binaries in the Age of the Next Generation of Large (Space) Telescopes

dc.creatorOlling, Rob P.
dc.date2005-05-23
dc.date.accessioned2026-07-07T02:17:40Z
dc.date.available2026-07-07T02:17:40Z
dc.descriptionI analyze several catalogs of known visual and spectroscopic binaries and conclude that a large number of binaries is missing in current catalogs. Samples of the best studied (nearby and bright) stars indicate that the true binary fraction may be as high as 95%. A preliminary analysis indicates that these binaries can a ect the astrometry signicantly.
dc.description4 pages, 2 figures To be published in: "Astrometry in the Age of the Next Generation of Large Telescopes," ASP Conference Series, 2005, Eds., P. Kenneth Seidelmann and Alice K. B. Monet
dc.identifierhttps://arxiv.org/abs/astro-ph/0505471
dc.identifierhttp://arxiv.org/abs/astro-ph/0505471
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9255
dc.subjectAstrophysics
dc.titleAstrometric Binaries in the Age of the Next Generation of Large (Space) Telescopes
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