NATURE OF RADIO AND OPTICAL EMISSIONS FROM PULSARS

被引：25

作者：

CHIU, HY

CANUTO, V

FASSIOCA.L

机构：

[1] Institute of Space Studies, New York, NY 10025

[2] Department of Earth and Space Sciences, State University of New York, Stony Brook

来源：

NATURE | 1969年 / 221卷 / 5180期

关键词：

D O I：

10.1038/221529a0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

A report of how rotating and oscillating magnetic neutron stars can account for the radio and optical signals from pulsars. Several predictions of the nature of the signals are put forward. © 1969 Nature Publishing Group.

引用

页码：529 / &

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CANUTO, V ;

CHIU, HY .

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[3] THERMODYNAMIC PROPERTIES OF A MAGNETIZED FERMI GAS [J].

CANUTO, V ;

CHIU, HY .

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[4] QUANTUM THEORY OF AN ELECTRON GAS IN INTENSE MAGNETIC FIELDS [J].

CANUTO, V ;

CHIU, HY .

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[5]

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[6]

CHIU HY, IN PRESS

[7]

COCKE WJ, 1969, IAU2128 CIRC

[8]

LYNDS R, IN PRESS

[9] PULSARS [J].

MARAN, SP ;

CAMERON, AGW .

PHYSICS TODAY, 1968, 21 (08) :41-&

[10]

Minkowski R, 1942, ASTROPHYS J, V96, P199, DOI 10.1086/144447

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