ROTATING NEUTRON STARS AND PULSAR EMISSION

被引：19

作者：

BERTOTTI, B

CAVALIERE, A

PACINI, F

机构：

[1] European Space Research Institute, Frascati

[2] Laboratorio Gas Lonizzati, Euratom, CNEN, Frascati

[3] Laboratorio di Astrofsica, Frascati

来源：

NATURE | 1969年 / 221卷 / 5181期

关键词：

D O I：

10.1038/221624a0

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：

The oblique rotator model of a neutron star can provide a mechanism to transfer rotational energy into the circumstellar plasma, producing periodic shock waves. This mechanism is also relevant to the activity sometimes observed in supernovae remnants. © 1969 Nature Publishing Group.

引用

页码：624 / +

页数：1

共 13 条

[1]

BUNEMAN O, 1962, J NUCL ENERGY, V4, pR3

[2]

Deutsch A. J., 1955, ANN ASTROPHYS, V18, P1

[3] SECOND PERIODIC PULSATION IN PULSARS [J].