A NEW CH-STAR IN OMEGA-CENTAURI

被引：8

作者：

COWLEY, AP

CRAMPTON, D

机构：

[1] ARIZONA STATE UNIV,DEPT PHYS,TEMPE,AZ 85287

[2] DOMINION ASTROPHYS OBSERV,VICTORIA V8X 4M6,BC,CANADA

来源：

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC | 1985年 / 97卷 / 595期

关键词：

D O I：

10.1086/131610

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：835 / 837

页数：3

共 20 条

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[6]

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[7]

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[8] FURTHER SPECTROSCOPIC EVIDENCE BEARING ON THE M22-OMEGA CENTAURI COMPARISON [J].

HESSER, JE ;

HARRIS, GLH .

ASTROPHYSICAL JOURNAL, 1979, 234 (02) :513-520

[9] CYANOGEN STRENGTHS AND UV EXCESSES OF EVOLVED STARS IN 17 GLOBULAR CLUSTERS FROM DDO PHOTOMETRY [J].

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[10] The spectra of CH stars [J].

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