POSSIBLE PRODUCTION OF SOFT-X-RAY BACKGROUND BY CORONAE OF RED GIANTS

被引：0

作者：

HILLS, JG ^{[1
]}

机构：

[1] UNIV MICHIGAN,DEPT ASTRON,ANN ARBOR,MI 48104

来源：

ASTROPHYSICAL LETTERS & COMMUNICATIONS | 1973年 / 14卷 / 01期

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：

引用

页码：69 / 71

页数：3

共 10 条

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[3] GALACTIC ORIGIN FOR SOFT-X-RAY BACKGROUND [J].

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TUCKER, WH .

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[4]

HILLS JG, 1973, ASTROPHYS LETT COMM, V13, P65

[5]

HILLS JG, 1972, ASTROPHYS LETT COMM, V12, P153

[6]

JOHNSON H, 1965, ANNU REV ASTRON ASTR, V4, P201

[7]

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[8]

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[9] X-RAY-EMISSION FROM WHITE DWARFS [J].

STRITTMATTER, PA ;

BRECHER, K ;

BURBIDGE, GR .

ASTROPHYSICAL JOURNAL, 1972, 174 (01) :91-+

[10] POSITIVE DETECTION OF AN EXCESS OF LOW-ENERGY DIFFUSE X-RAYS AT HIGH GALACTIC LATITUDE [J].

YENTIS, DJ ;

VANDENBO.P ;

NOVICK, R .

ASTROPHYSICAL JOURNAL, 1972, 177 (02) :365-&

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