G308.8-0.1 - AN UNUSUAL SUPERNOVA REMNANT CONTAINING A SHORT-PERIOD PULSAR, PSR-J1341-6220

被引：29

作者：

CASWELL, JL

KESTEVEN, MJ

STEWART, RT

MILNE, DK

HAYNES, RF

机构：

[1] Australian Telescope Natl. Facility, CSIRO, Epping, NSW 2121

来源：

ASTROPHYSICAL JOURNAL | 1992年 / 399卷 / 02期

关键词：

PULSARS; INDIVIDUAL; (PSR-J1341-6220); SUPERNOVA REMNANTS;

D O I：

10.1086/186629

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Galactic radio source G308.8-0.1 is a supernova remnant shell of which the brightest part, G308.7+0.0, was formerly cataloged as a supernova remnant in its own right. The shell, as now defined by sensitive new observations, contains a short-period pulsar within its boundary. Both are probably relics of the same supernova event.

引用

页码：L151 / L153

页数：3

共 16 条

[1] GALACTIC SUPER-NOVA REMNANTS - DEPENDENCE OF RADIO BRIGHTNESS ON GALACTIC HEIGHT AND ITS IMPLICATIONS [J].