Searching for star-planet magnetic interaction in CoRoT observations

被引：14
作者：
Lanza, A. F. [1 ]
机构：
[1] INAF Osservatorio Astrofis Catania, I-95123 Catania, Italy
来源：
ASTROPHYSICS AND SPACE SCIENCE | 2011年 / 336卷 / 02期
关键词：
Stars: planetary systems; Stars: activity; Stars: late-type; Stars: magnetic fields; Stars: general; EXTRASOLAR GIANT PLANETS; CLOSE BINARY STARS; HOT JUPITERS; DIFFERENTIAL ROTATION; CHROMOSPHERIC ACTIVITY; PHOTOSPHERIC ACTIVITY; STELLAR ACTIVITY; RADIO-EMISSION; FLUX TUBES; SHORT-TERM;
D O I：
10.1007/s10509-011-0878-4
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Close-in massive planets interact with their host stars through tidal and magnetic mechanisms. In this paper, we review circumstantial evidence for star-planet interaction as revealed by the photospheric magnetic activity in some of the CoRoT planet-hosting stars, notably CoRoT-2, 4, and 6. The phenomena are discussed in the general framework of activity-induced features in stars accompanied by hot Jupiters. The theoretical mechanisms proposed to explain the activity enhancements possibly related with hot Jupiters are also briefly reviewed with an emphasis on the possible effects at the photospheric level. The unique advantages of CoRoT and Kepler observations to test these models are pointed out.
引用
收藏
页码：303 / 313
页数：11
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