X-ray emission properties of rotation-driven pulsars

被引：5

作者：

Becker, W ^{[1
]}

机构：

[1] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany

来源：

BROAD BAND X-RAY SPECTRA OF COSMIC SOURCES | 2000年 / 25卷 / 3-4期

关键词：

D O I：

10.1016/S0273-1177(99)00817-0

中图分类号：

V [航空、航天];

学科分类号：

08 [工学]; 0825 [航空宇航科学与技术];

摘要：

Recent X-ray observatories like ROSAT, ASCA, BeppoSax and RXTE have achieved important progress in neutron star and pulsar astronomy. The identification of Geminga, the discovery of X-ray emission from millisecond pulsars and the identification of cooling neutron stars are only few of the fascinating results. In the following we will give a brief review on the X-ray emission properties of rotation-powered pulsars and their wind nebulae as observed by these instruments. (C) 2000 COSPAR. Published by Elsevier Science Ltd.

引用

页码：647 / 658

页数：12

共 32 条

[1]

Becker W, 1997, ASTRON ASTROPHYS, V326, P682

[2]

Becker W, 1999, ASTRON ASTROPHYS, V341, P803

[3]

Becker W, 1996, ASTRON ASTROPHYS SUP, V120, pC69

[4]

BECKER W, 1995, NATO ADV SCI INST SE, V450, P47

[5]

BECKER W, 1999, UNPUB

[6]

High-resolution X-ray imaging of the supernova remnant MSH 15-52 [J].

Brazier, KTS ;

Becker, W .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 284 (02) :335-340

[7]

Faint X-ray sources in the core of the globular cluster M28 [J].

Danner, R ;

Kulkarni, SR ;

Saito, Y ;

Kawai, N .

NATURE, 1997, 388 (6644) :751-753

[8]

DAVID LP, 1997, ROSAT HRI CALIBRATIO

[9]

GAENSLER BM, 1998, WORKSH REL NEUTR STA

[10]

An unusual X-ray burst from the globular cluster M28 [J].

Gotthelf, EV ;

Kulkarni, SR .

ASTROPHYSICAL JOURNAL, 1997, 490 (02) :L161-&

← 1 2 3 4 →