SOLAR MODELS OF LOW NEUTRINO-COUNTING RATE - DEPLETED MAXWELLIAN TAIL

被引：45

作者：

CLAYTON, DD ^{[1
]}

DWEK, E ^{[1
]}

NEWMAN, MJ ^{[1
]}

TALBOT, RJ ^{[1
]}

机构：

[1] RICE UNIV,DEPT SPACE PHYS & ASTRON,HOUSTON,TX 77001

来源：

ASTROPHYSICAL JOURNAL | 1975年 / 199卷 / 02期

关键词：

D O I：

10.1086/153715

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：494 / 499

页数：6

共 11 条

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[3]

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[4]

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[5] MAXWELLIAN RELATIVE ENERGIES AND SOLAR NEUTRINOS [J].

CLAYTON, DD .

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[6]

COX JP, 1968, PRINCIPLES STELLAR S, pCH20

[7] INTERNAL STRUCTURE OF MIDDLE MAIN-SEQUENCE STARS [J].

IBEN, I ;

EHRMAN, JR .

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[8] CENTRAL CONVECTION AND SOLAR NEUTRINOS [J].

IBEN, I .

ASTROPHYSICAL JOURNAL, 1969, 155 (2P2) :L101-&

[9]

KOCHAROV GE, 1972, 298 IOFF PHYS TECHN

[10]

NEWMAN MJ, 1975, THESIS RICE U

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