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.

引用

页码：435 / 442

页数：7

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