Radio and X-ray emission associated with the supernova remnant G352.7-0.1

被引：0

作者：

Giacani, E ^{[1
]}

Loiseau, N

Dubner, G

Smith, MJS

机构：

[1] Inst Astron & Space Phys, Buenos Aires, DF, Argentina

[2] ESAC, XMM Newton Sci Operat Ctr, Villaffanca del Castillo, France

来源：

PROCEEDINGS OF THE X-RAY UNIVERSE 2005, VOLS 1 AND 2 | 2006年 / 604卷

关键词：

X-rays; radio continuum; supernova remnants; G352.7-0.1; ISM;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report on new VLA radio and XMM-Newton X-ray observations of the SNR G352.7-0.1. These high sensitivity, high resolution data reveal that G352.7-0.1 belongs to the thermal composite morphological class. Small scale structures in radio and X-ray emission are not always correlated and are different for the different X-rays bands examined. The distance to G352.7-0.1 can be constrained between 6.6 and 8.4 kpc. The study of the HI suggests that G352.7-0.1 is located within a cavity probably created by the stellar wind of the precursor star.

引用

页码：367 / +

页数：2

共 6 条

[1] ABUNDANCES OF THE ELEMENTS - METEORITIC AND SOLAR [J].