A DISTANCE DETERMINATION FOR THE SUPERNOVA REMNANT G27.4+0.0 AND ITS CENTRAL X-RAY SOURCE

被引：43

作者：

SANBONMATSU, KY

HELFAND, DJ

机构：

[1] Columbia Astrophysics Laboratory, Columbia University, New York

来源：

ASTRONOMICAL JOURNAL | 1992年 / 104卷 / 06期

关键词：

D O I：

10.1086/116393

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have determined the distance to the supernova remnant G27.4+0.0, one of the handful of remnants with a bright central x-ray source. H I absorption data obtained with the VLA toward the remnant and adjacent H II regions allow us to constrain the distance to G27.4+0.0 to lie between 6 and 7.5 kpc. We briefly discuss the implications of this result for the nature of the central source.

引用

页码：2189 / 2192

页数：4

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