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 / &

共 10 条

[1] The Crab nebula
Baade, W
[J]. ASTROPHYSICAL JOURNAL, 1942, 96 (02) : 188 - 198
[2] MAGNETIC MOMENT OF A MAGNETIZED FERMI GAS
CANUTO, V
CHIU, HY
[J]. PHYSICAL REVIEW, 1968, 173 (05): : 1229 - &
[3] THERMODYNAMIC PROPERTIES OF A MAGNETIZED FERMI GAS
CANUTO, V
CHIU, HY
[J]. PHYSICAL REVIEW, 1968, 173 (05): : 1220 - &
[4] QUANTUM THEORY OF AN ELECTRON GAS IN INTENSE MAGNETIC FIELDS
CANUTO, V
CHIU, HY
[J]. PHYSICAL REVIEW, 1968, 173 (05): : 1210 - &
[5] CANUTO V, IN PRESS
[6] CHIU HY, IN PRESS
[7] COCKE WJ, 1969, IAU2128 CIRC
[8] LYNDS R, IN PRESS
[9] PULSARS
MARAN, SP
CAMERON, AGW
[J]. PHYSICS TODAY, 1968, 21 (08) : 41 - &
[10] Minkowski R, 1942, ASTROPHYS J, V96, P199, DOI 10.1086/144447

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