A NEW METHOD TO OPTIMIZE PARAMETERS IN SOLUTIONS OF ECLIPSING BINARY LIGHT CURVES

被引：70

作者：

KALLRATH, J ^{[1
]}

LINNELL, AP ^{[1
]}

机构：

[1] MICHIGAN STATE UNIV,DEPT PHYS & ASTRON,E LANSING,MI 48824

来源：

关键词：

D O I：

10.1086/164971

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：346 / 357

页数：12

共 23 条

[1]

CACECI MS, 1984, BYTE, V9, P340

[2] A UBV PHOTOMETRIC STUDY OF MR-CYGNI [J].

HALL, DS ;

HARDIE, RH .

[3]

HILL G, 1972, ASTR AP, V23, P357

[4] IMAGES OF ACCRETION DISKS .1. THE ECLIPSE MAPPING METHOD [J].

HORNE, K .

[5]

Khaliullina A. I., 1984, Soviet Astronomy, V28, P228

[6] A LIGHT SYNTHESIS PROGRAM FOR BINARY STARS .1. [J].

LINNELL, AP .

[7]

LINNELL AP, 1972, AP J SUPPL, V24, P449

[8]

LINNELL AP, 1970, AP J, V162, P162

[9] SIMPLEX OPTIMIZATION OF RESPONSE FROM CHEMICAL SYSTEMS [J].

LONG, DE .

[10]

MURRAY W, 1972, NUMERICAL METHODS UN