X-ray gaseous emission in star forming galaxies

被引：1
|
作者：
Ranalli, Piero [1 ]
Comastri, Andrea [2 ]
Origlia, Livia [2 ]
Maiolino, Roberto [3 ]
机构：
[1] Univ Bologna, Via Ranzani 1, I-40127 Bologna, Italy
[2] Osservatorio Astron Bologna, INAF, I-40127 Bologna, Italy
[3] Osserv Astron Roma, INAF, I-00040 Monte Porzio Catone, Italy
来源：
X-RAY ASTRONOMY-2009: PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES, PROCEEDINGS | 2010年 / 1248卷
关键词：
galaxies: individual: M82; galaxies: abundances; X-rays: ISM; plasmas; atomic processes; GALACTIC RIDGE; ORIGIN; M82;
D O I：
10.1063/1.3475218
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The main results from a deep X-ray observation of M82 are summarised: spatially-dependent chemical abundances, temperature structure of the gas, charge-exchange emission lines in the spectrum. We also present an update of the chemical abundances, based on a more refined extraction of spectra.
引用
收藏
页码：229 / +
页数：2
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