HIGH-FREQUENCY OPTICAL VARIABLES .2. LUMINOSITY-VARIABLE WHITE-DWARFS AND MAXIMUM ENTROPY SPECTRAL ANALYSIS

被引：35

作者：

RICHER, HB ^{[1
]}

ULRYCH, TJ ^{[1
]}

机构：

[1] UNIV BRITISH COLUMBIA,DEPT GEOPHYS & ASTRON,2075 WESBROOK PL,VANCOUVER V6T 1W5,BRITISH COLUMBI,CANADA

来源：

关键词：

D O I：

10.1086/153110

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：719 / 730

页数：12

共 34 条

[1]

ABELS JG, 1972, S COLLECTION ANALYSI

[2] POWER SPECTRUM ESTIMATION THROUGH AUTOREGRESSIVE MODEL FITTING [J].

AKAIKE, H .

[3] STATISTICAL PREDICTOR IDENTIFICATION [J].

AKAIKE, H .

[4]

AKAIKE H, 1969, ANN I STAT MATH, V21, P261

ANDERSEN, N .

[6]

Blackman R.B., 1958, MEASUREMENT POWER SP

[7] On the mechanism of accretion by stars [J].

Bondi, H ;

Hoyle, F .

[8]

BRILLOUIN L, 1956, SCIENCE INFORMATION

[9]

Burg J.P., 1967, 37 ANN INT SOC EXPL

[10]

BURG JP, 1968, NATURE, V236, P83