Element Abundances in X-ray Emitting Plasmas in Stars

被引:23
|
作者
Testa, Paola [1 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
关键词
Element abundances; X-rays; Spectroscopy; Stars; X-ray activity; STELLAR CORONAL ABUNDANCES; T-TAURI STARS; PHOTOSPHERIC ABUNDANCES; SOLAR NEIGHBORHOOD; ZETA-PUPPIS; SPECTROSCOPY; EMISSION; FLARE; NEON; ACCRETION;
D O I
10.1007/s11214-010-9714-3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Studies of element abundances in stars are of fundamental interest for their impact in a wide astrophysical context, from our understanding of galactic chemistry and its evolution, to their effect on models of stellar interiors, to the influence of the composition of material in young stellar environments on the planet formation process. We review recent results of studies of abundance properties of X-ray emitting plasmas in stars, ranging from the corona of the Sun and other solar-like stars, to pre-main sequence low-mass stars, and to early-type stars. We discuss the status of our understanding of abundance patterns in stellar X-ray plasmas, and recent advances made possible by accurate diagnostics now accessible thanks to the high resolution X-ray spectroscopy with Chandra and XMM-Newton.
引用
收藏
页码:37 / 55
页数:19
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