TODCOR - Two-Dimensional Correlation

被引:0
|
作者
Zucker, Shay [1 ]
机构
[1] Tel Aviv Univ, Raymond & Beverly Sackler Fac Exact Sci, Dept Geophys & Planetary Sci, IL-69978 Tel Aviv, Israel
来源
FROM INTERACTING BINARIES TO EXOPLANETS: ESSENTIAL MODELING TOOLS | 2012年 / 282期
关键词
Celestial mechanics; methods: data analysis; techniques: radial velocities; techniques: spectroscopic; binaries: spectroscopic; stars: low mass; brown dwarfs; planetary systems; CROSS-CORRELATION; BINARY STARS; HARO; 1-14C; PLANET;
D O I
10.1017/S1743921311027852
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
TODCOR is a TwO-Dimensional CORrelation technique to measure radial velocities of the two components of a spectroscopic binary. Assuming the spectra of the two components are known, the technique correlates an observed binary spectrum against a combination of the two spectra with different shifts. TODCOR measures simultaneously the radial velocities of the two stars by finding the maximum correlation. The main use of the technique has been to turn single-lined binaries into double-lined systems. This helps to explore the binary mass-ratio distribution, especially the low-mass regime, where the secondaries are usually very faint and therefore hard to detect. The technique has been generalized to study multi-order spectra, and also triple- and quadruple-lined systems. It has several applications in studying extrasolar planets and in the future may even help to dynamically measure stellar masses of binaries through relativistc effects.
引用
收藏
页码:371 / 378
页数:8
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