Speckle interferometry of secondary components in nearby visual binaries

Resource type
Authors/contributors
Title
Speckle interferometry of secondary components in nearby visual binaries
Abstract
Statistical characterization of secondary subsystems in binaries helps to distinguish between various scenarios of multiple-star formation. The Differential Speckle Survey Instrument was used at the Gemini-N telescope for several hours in 2015 July to probe the binarity of 25 secondary components in nearby solar-type binaries. Six new subsystems were resolved, with meaningful detection limits for the remaining targets. The large incidence of secondary subsystems agrees with other similar studies. The newly resolved subsystem HIP 115417 Ba,Bb causes deviations in the observed motion of the outer binary from which an astrometric orbit of Ba,Bb with a period of 117 years is deduced. © 2016. The American Astronomical Society. All rights reserved.
Publication
The Astronomical Journal
Date
2016
Volume
152
Issue
5
Pages
116
Journal Abbr
Astron. J.
Citation Key
pop00287
ISSN
00046256 (ISSN)
Language
English
Extra
17 citations (Crossref) [2023-10-31] Citation Key Alias: lens.org/112-209-617-018-947 tex.type: [object Object]
Citation
Tokovinin, A., & Horch, E. P. (2016). Speckle interferometry of secondary components in nearby visual binaries. The Astronomical Journal, 152(5), 116. https://doi.org/10.3847/0004-6256/152/5/116