ICCD speckle observations of binary stars: Measurements during 1994-1995

被引:16
作者
Aristidi, E
Carbillet, M
Prieur, JL
Lopez, B
Bresson, Y
Koechlin, L
机构
[1] Univ Nice Sophia, CNRS, UMR 6525, F-06108 Nice 2, France
[2] Observ Midi Pyrenees, F-31000 Toulouse, France
[3] Observ Cote Azur, Dept Fresnel, UMR 6528, F-06304 Nice 4, France
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1997年 / 126卷 / 03期
关键词
methods; data analysis; techniques; image processing; interferometric; binaries; close;
D O I
10.1051/aas:1997282
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present speckle observations of nineteen double stars and the triple star 2 Cam. Angular separations, absolute position angles and relative photometry result from these observations. The angular separation is derived from the power spectrum. The position angle and the relative photometry are determined by two recent techniques: the cross-correlation between the speckle images and their square, and the ratios of twofold probability density functions of the images.
引用
收藏
页码:555 / 561
页数:7
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