Diffuse X-ray emission from the Magellanic Clouds

被引：0

作者：

Sasaki, M ^{[1
]}

Haberl, F ^{[1
]}

Pietsch, W ^{[1
]}

机构：

[1] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany

来源：

X-RAY ASTRONOMY 2000 | 2001年 / 234卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The diffuse X-ray emission in the Magellanic Clouds is studied using all pointed observations of the ROSAT PSPC. Contributions from the distinct sources listed in the ROSAT HRI and PSPC source catalogues were eliminated and periods of high solar activity were excluded. PSPC spectra were analyzed for 0.25degrees x 0.25degrees regions both in the SMC and the LMC yielding characteristic temperatures of 10(6) - 10(7) K for the diffuse emission in the MCs. The spatial variation is compared to the distribution of SNRs in the MCs. In. addition, new results from an XMM-Newton EPIC-PN observation of diffuse emission close to the 30 Doradus region are discussed.

引用

页码：319 / 324

页数：6

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