| Issue |
A&A
Volume 415, Number 1, February III 2004
|
|
|---|---|---|
| Page(s) | 259 - 264 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20034069 | |
| Published online | 03 February 2004 | |
Orbits of 10 interferometric binary systems calculated by using the improved Koval'skij method*
1
Astronomical Observatory, Volgina 7, 11160-Belgrade 74, Serbia and Montenegro
2
Institute Isaac Newton of Chile, Yugoslavia Branch
Corresponding author: D. Olević, dolevic@aob.bg.ac.yu
Received:
11
July
2003
Accepted:
4
October
2003
Orbital elements are presented of 10 interferometric binary systems with no previous orbit determination: WDS 07143–2621 (FIN 323), WDS 12064–6543 (FIN 367Aa), WDS 12446–5717 (FIN 65), WDS 13320–6519 (FIN 369), WDS 13574–6229 (FIN 370), WDS 14189+5452 (CHR 137), WDS 14373–4608 (FIN 318 Aa), WDS 16115+0943 (FIN 354), WDS 17018–5108 (I 1306), WDS 17221–7007 (FIN 373). The method used (Koval'skij-Olević) is briefly described.
Key words: techniques: interferometric / stars: binaries: close
© ESO, 2004
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