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Issue A&A
Volume 384, Number 1, March II 2002
Page(s) 171 - 179
Section Formation, structure and evolution of stars
DOI http://dx.doi.org/10.1051/0004-6361:20011805



A&A 384, 171-179 (2002)
DOI: 10.1051/0004-6361:20011805

Orbits for five southern visual binaries

R. W. Argyle1, A. Alzner2 and E. P. Horch3

1  Institute of Astronomy, Madingley Road, Cambridge CB3 0HA, UK
2  Zeckerner Hauptstrasse 3, 91334 Hemhofen, Germany
    e-mail: Aalzner@aol.com
3  Chester F. Carlson Center for Imaging Science, Rochester Institute of Technology, 54 Lomb Memorial Drive, Rochester, NY 14623-5604, USA
    e-mail: horch@cis.rit.edu

(Received 16 July 2001 / Accepted 18 December 2001 )

Abstract
First orbits have been calculated for the visual binaries WDS 00090-5400, 01061-4643, 05248-5219 and 08447-5443 (Alzner & Argyle 2000; Argyle & Alzner 2000). The current period for the orbit of (Wierzbinski 1958) is too short to represent recent observations. The period has been lengthened to 450 years (Alzner & Argyle 2001). For 00090-5400 the period is 221 years with a moderate eccentricity; 01061-4643 is currently near periastron but is underobserved; 05248-5219 has passed periastron but there have been no observations since 1993. The visual component of WDS 08447-5443 (= $\delta$ Vel), which is not the same as the eclipsing component recently discovered by Otero (2000), has an unexpectedly short period.


Key words: astrometry -- binaries: close -- binaries: visual -- techniques: interferometric

Offprint request: R. W. Argyle, rwa@ast.cam.ac.uk

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