X-ray variability of cool stars: Magnetic activity and accretion

被引：6
作者：
Stelzer, B. [1 ]
机构：
[1] INAF Osservatorio Astron Palermo, Piazza Parlamento 1, I-90134 Palermo, Italy
来源：
ASTRONOMISCHE NACHRICHTEN | 2017年 / 338卷 / 2-3期
关键词：
X-rays: stars; stars: late-type; stars: pre-main sequence; stars: activity; stars: coronae; T-TAURI STARS; XMM-NEWTON OBSERVATION; YOUNG STELLAR OBJECTS; ORION NEBULA CLUSTER; MAIN-SEQUENCE STARS; ROTATIONAL MODULATION; ALPHA CENTAURI; SOLAR-FLARES; CORONAL STRUCTURE; DISK INTERACTION;
D O I：
10.1002/asna.201713330
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
This article provides a review of X-ray variability from late-type stars with particular focus on the achievements of XMM-Newton and its potential for future studies in this field.
引用
收藏
页码：195 / 200
页数：6
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