ESTIMATION OF BINARY STAR PARAMETERS BY MODEL-FITTING THE BISPECTRUM PHASE

被引：10

作者：

GLINDEMANN, A

LANE, RG

DAINTY, JC

机构：

[1] Optics Section, Blackett Laboratory, Imperial College, London

来源：

JOURNAL OF THE OPTICAL SOCIETY OF AMERICA A-OPTICS IMAGE SCIENCE AND VISION | 1992年 / 9卷 / 04期

关键词：

D O I：

10.1364/JOSAA.9.000543

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The analysis of binary stars has to date been one of the major successes of speckle interferometry. A new technique for estimating the parameters of a binary star is presented. Unlike earlier methods, the system does not require the measurement of a reference star to compensate for the speckle transfer function. The algorithm relies on model fitting to the bispectrum phase and can obtain the separation, position angle, and relative brightness of the two components.

引用

页码：543 / 548

页数：6

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