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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. Horch31 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 (=
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
SIMBAD Objects
© ESO 2002
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