Disk Wind in the Radiation of Two Herbig Ae/Be Stars: MWC 480 and IL Cep

被引:0
|
作者
Grinin, V. [1 ,2 ]
Tambovtseva, L. [1 ]
Potravnov, I. [1 ]
Mkrtichian, D. [3 ]
机构
[1] Russian Acad Sci, Pulkovo Astron Observ, Pulkovskoe Shosse 65, St Petersburg 196140, Russia
[2] St Petersburg State Univ, Sobolev Astron Inst, Univ Skii Pr 28, St Petersburg 198504, Russia
[3] Nat Astron Res Inst Thailand, Chiang Mai 50200, Thailand
来源
B(E) PHENOMENON: FORTY YEARS OF STUDIES | 2017年 / 508卷
基金
俄罗斯基础研究基金会;
关键词
PRE-MAIN-SEQUENCE; YOUNG STARS; ACCRETION; EMISSION; FLOWS; MAGNETOSPHERE; VARIABILITY; MODEL;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using non-LTE modeling for different components of the curcumstellar environment in Herbig AeBe stars, we reproduced hydrogen emission lines, such as Ha and H beta, and determined geometrical and physical parameters of the line emitting regions. Two Herbig stars (MWC 480 and IL Cep) have been considered. The modeling shows that the disk wind or X-wind are the main contributors to the radiation of the lines of the Balmer series compared to the magnetospheric accreting region.
引用
收藏
页码:185 / 189
页数:5
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