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

被引：44

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：

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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BAHCALL, JN
ULRICH, RK
[J]. ASTROPHYSICAL JOURNAL, 1971, 170 (03) : 593 - &
[2] SENSITIVITY OF SOLAR-NEUTRINO FLUXES
BAHCALL, JN
BAHCALL, NA
ULRICH, RK
[J]. ASTROPHYSICAL JOURNAL, 1969, 156 (2P1) : 559 - &
[3] CAMERON AGW, 1973, EXPLOSIVE NUCLEOSYNT
[4] Clayton D. D., 1968, PRINCIPLES STELLAR E
[5] MAXWELLIAN RELATIVE ENERGIES AND SOLAR NEUTRINOS
CLAYTON, DD
[J]. NATURE, 1974, 249 (5453) : 131 - 131
[6] COX JP, 1968, PRINCIPLES STELLAR S, pCH20
[7] INTERNAL STRUCTURE OF MIDDLE MAIN-SEQUENCE STARS
IBEN, I
EHRMAN, JR
[J]. ASTROPHYSICAL JOURNAL, 1962, 135 (03) : 770 - &
[8] CENTRAL CONVECTION AND SOLAR NEUTRINOS
IBEN, I
[J]. ASTROPHYSICAL JOURNAL, 1969, 155 (2P2) : L101 - &
[9] KOCHAROV GE, 1972, 298 IOFF PHYS TECHN
[10] NEWMAN MJ, 1975, THESIS RICE U