RADIO EMISSION FROM MAGNETIC NEUTRON STARS - A POSSIBLE MODEL FOR PULSARS

被引：25

作者：

CHIU, HY

CANUTO, V

机构：

[1] Goddard Institute for Space Studies, New York

来源：

PHYSICAL REVIEW LETTERS | 1969年 / 22卷 / 09期

关键词：

D O I：

10.1103/PhysRevLett.22.415

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We show that radio emission from a neutron star with a magnetic field of 109 G or more can account for the radio emission of pulsars. It is suggested that pulsars also emit two bands, one in the uv or optical, and the other in the infrared in the decamicron wavelength range. © 1969 The American Physical Society.

引用

页码：415 / &

共 25 条

[1] MAGNETIC MOMENT OF A MAGNETIZED FERMI GAS [J].

CANUTO, V ;

CHIU, HY .

PHYSICAL REVIEW, 1968, 173 (05) :1229-&

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

CANUTO, V ;

CHIU, HY .

PHYSICAL REVIEW, 1968, 173 (05) :1220-&

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

CANUTO, V ;

CHIU, HY .

PHYSICAL REVIEW, 1968, 173 (05) :1210-&

[4]

CANUTO V, TO BE PUBLISHED

[5] SUPERNOVAE, NEUTRINOS, AND NEUTRON STARS [J].

CHIU, HY .

ANNALS OF PHYSICS, 1964, 26 (03) :364-410

[6] PROBLEMS OF INTENSE MAGNETIC FIELD IN GRAVITATIONAL COLLAPSE [J].

CHIU, HY ;

CANUTO, V .

ASTROPHYSICAL JOURNAL, 1968, 153 (3P2) :L157-&

[7] SURFACE X-RAY EMISSION FROM NEUTRON STARS [J].

CHIU, HY ;

SALPETER, EE .

PHYSICAL REVIEW LETTERS, 1964, 12 (15) :413-+

[8]

CHIU HY, TO BE PUBLISHED

[9]

CHIU HY, 1968, STELLAR PHYSICS, P217

[10]

CHIU HY, 1969, PHYS REV, V176, P1438

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