Volume 415, Number 1, February III 2004
|Page(s)||259 - 264|
|Section||Stellar structure and evolution|
|Published online||03 February 2004|
Orbits of 10 interferometric binary systems calculated by using the improved Koval'skij method*
Astronomical Observatory, Volgina 7, 11160-Belgrade 74, Serbia and Montenegro
2 Institute Isaac Newton of Chile, Yugoslavia Branch
Corresponding author: D. Olević, firstname.lastname@example.org
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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