Velocity curve analysis of the spectroscopic binary stars by the non-linear least squares

被引：0
作者：
K. Karami
H. Teimoorinia
机构：
[1] University of Kurdistan,Department of Physics
[2] Research Institute for Astronomy & Astrophysics of Maragha (RIAAM),undefined
[3] Institute for Advanced Studies in Basic Sciences (IASBS),undefined
[4] Gava Zang,undefined
[5] Institute for Advanced Studies in Basic Sciences (IASBS),undefined
[6] Gava Zang,undefined
[7] Islamic Azad University-Zanjan,undefined
来源：
Astrophysics and Space Science | 2007年 / 311卷
关键词：
Spectroscopic binary stars; Eclipsing binary stars;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
We introduce a new method to derive the orbital parameters of spectroscopic binary stars by a non-linear least squares analysis of residuals. Using measured radial velocity data of four double lined spectroscopic binary systems RZ Cas, CC Cas, V1130 Tau and Y Cygni, we find corresponding orbital and spectroscopic elements. Our numerical results are in good agreement with those obtained by others using more traditional methods.
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页码：435 / 442
页数：7
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