Speckle spectroscopic observations of Be binary stars

被引：0

作者：

Baba, N ^{[1
]}

Kuwamura, S ^{[1
]}

Norimoto, Y ^{[1
]}

Cuevas, S ^{[1
]}

机构：

[1] Hokkaido Univ, Dept Appl Phys, Sapporo, Hokkaido 060, Japan

来源：

THIRD PACIFIC RIM CONFERENCE ON RECENT DEVELOPMENT ON BINARY STAR RESEARCH | 1997年 / 130卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Be binary stars, phi And, lambda Cyg, and beta Mon have been observed by our speckle spectroscopic camera. Each spectrum of the primary and the secondary stars is spatially separated by the speckle spectroscopic method, which can resolve binary stars with diffraction-limited angular resolution of a telescope. The spectra around H alpha line are examined.

引用

页码：35 / 40

页数：4