Speckle Interferometry of Metal-Poor Stars in the Solar Neighborhood. I

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dc.creatorRastegaev, D. A.
dc.creatorBalega, Yu. Yu.
dc.creatorMalogolovets, E. V.
dc.date2007-07-19
dc.date2007-07-20
dc.date.accessioned2026-07-07T08:19:13Z
dc.date.available2026-07-07T08:19:13Z
dc.descriptionWe report the results of speckle-interferometric observations of 109 high proper-motion metal-poor stars made with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. We resolve eight objects -- G102-20, G191-55, BD+19$^\circ$~1185A, G89-14, G87-45, G87-47, G111-38, and G114-25 -- into individual components and we are the first to astrometrically resolve seven of these stars. New resolved systems included two triple (G111-38, G87-47) and one quadruple (G89-14) star. The ratio of single-to-binary-to-triple-to-quadruple systems among the stars of our sample is equal to 71:28:6:1.
dc.description8 pages, 4 figures, accepted to Astrophysical Bulletin
dc.identifierhttps://arxiv.org/abs/0707.2903
dc.identifierhttp://arxiv.org/abs/0707.2903
dc.identifierdoi:10.1134/S1990341307030042
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/134694
dc.subjectAstrophysics
dc.titleSpeckle Interferometry of Metal-Poor Stars in the Solar Neighborhood. I
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