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Proceedings Paper

Initial scientific results from phase-referenced astrometry of sub-arcsecond binaries
Author(s): Matthew W. Muterspaugh; Benjamin F. Lane; Bernard F. Burke; Maciej Konacki; Shri R. Kulkarni
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Paper Abstract

The Palomar Testbed Interferometer has observed several binary star systems whose separations fall between the interferometric coherence length (a few hundredths of an arcsecond) and the typical atmospheric seeing limit of one arcsecond. Using phase-referencing techniques we measure the relative separations of the systems to precisions of a few tens of micro-arcseconds. We present the first scientific results of these observations, including the astrometric detection of the faint third stellar component of the kappa Pegasi system.

Paper Details

Date Published: 20 October 2004
PDF: 8 pages
Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); doi: 10.1117/12.551980
Show Author Affiliations
Matthew W. Muterspaugh, Massachusetts Institute of Technology (United States)
Benjamin F. Lane, Massachusetts Institute of Technology (United States)
Bernard F. Burke, Massachusetts Institute of Technology (United States)
Maciej Konacki, California Institute of Technology (United States)
Shri R. Kulkarni, California Institute of Technology (United States)

Published in SPIE Proceedings Vol. 5491:
New Frontiers in Stellar Interferometry
Wesley A. Traub, Editor(s)

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