Stellar coronae with XMM-Newton RGS II.: X-ray variability

被引：0

作者：

Audard, M ^{[1
]}

Güdel, M ^{[1
]}

den Boggende, AJ ^{[1
]}

Brinkman, AC ^{[1
]}

den Herder, JW ^{[1
]}

Kaastra, JS ^{[1
]}

Mewe, R ^{[1
]}

Raassen, AJJ ^{[1
]}

de Vries, C ^{[1
]}

Behar, E ^{[1
]}

Cottam, J ^{[1
]}

Kahn, SM ^{[1
]}

Paerels, FBS ^{[1
]}

Peterson, JM ^{[1
]}

Rasmussen, AP ^{[1
]}

Sako, M ^{[1
]}

Branduardi-Raymont, G ^{[1
]}

Sakelliou, I ^{[1
]}

Erd, C ^{[1
]}

机构：

[1] Paul Scherrer Inst, CH-5232 Villigen, Switzerland

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：

First results from high-resolution coronal spectroscopy of flares with the Reflection Grating Spectrometers on board the XMM-Newton satellite are reviewed. Rotational modulation in the X-ray light curve of HR 1099 is discussed. Results from time-dependent spectroscopy of flares in the active stars HR 1099, AB Dor, YY Gem are also presented. Variations in the shape of the emission measure distributions, in the abundances and in the average density of the cool plasma are discussed.

引用

页码：79 / 84

页数：6

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