Features of the Magnetic Field Behavior of the Ae/Be Star HD190073

被引：0
|
作者：
Glagolevskij, Yu. V. [1 ]
机构：
[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz, Russia
来源：
ASTROPHYSICS | 2023年 / 66卷 / 02期
关键词：
Ae; Be stars; HD190073; magnetic field; ORIENTATION; AXES;
D O I：
10.1007/s10511-023-09784-0
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
An attempt is made to explain the sudden change in the surface structure of the magnetic field of the type HAe/Be star HD190073 assuming a variable nonstationarity of the upper layers of the star which takes place owing to accretion and burning of deuterium. At the same time, data are presented which contradict the assumption of magnetic field generation within the convective core.
引用
收藏
页码：224 / 234
页数：11
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