UPPER LIMITS TO X-RAY-EMISSION FROM BETA-PERSEI DURING RADIO FLARES

被引：10

作者：

CANIZARES, CR

NEIGHBOURS, JE

CLARK, GW

LEWIN, WHG

SCHNOPPER, HW

SPROTT, GF

机构：

[1] MIT, DEPT PHYS, CAMBRIDGE, MA 02139 USA

[2] MIT, CTR SPACE RES, CAMBRIDGE, MA 02139 USA

来源：

ASTROPHYSICAL JOURNAL | 1973年 / 183卷 / 02期

关键词：

D O I：

10.1086/181259

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L91 / L93

页数：3

共 7 条

[1]

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[2]

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[4] BETA PERSEI - RADIO STAR AND PROBABLE X-RAY STAR [J].

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NATURE-PHYSICAL SCIENCE, 1972, 238 (82) :52-+

[5] RADIO BEHAVIOR OF BETA PERSEI [J].

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WEBSTER, E ;

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ASTROPHYSICAL JOURNAL, 1972, 178 (03) :L139-L144

[6] RADIO VARIATIONS OF BETA-PERSEI AND BETA-LYRAE [J].

HJELLMING, RM ;

WEBSTER, E ;

WADE, CM .

NATURE-PHYSICAL SCIENCE, 1972, 236 (64) :43-+

[7] POSSIBLE EXPLANATION FOR NONTHERMAL RADIO NOISE FROM BINARY STARS [J].

JONES, TW ;

WOOLF, NJ .

ASTROPHYSICAL JOURNAL, 1973, 179 (03) :869-873

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