T Tauri Stars in Taurus-Auriga Star-Forming Region: Reliable Interstellar Extinction

被引：0
|
作者：
Grankin, Konstantin N. [1 ]
机构：
[1] Crimean Astrophys Observ, Nauchny 298409, Crimea, Russia
来源：
NON-STABLE UNIVERSE: ENERGETIC RESOURCES, ACTIVITY PHENOMENA, AND EVOLUTIONARY PROCESSES | 2017年 / 511卷
基金：
俄罗斯基础研究基金会;
关键词：
TERM PHOTOMETRIC VARIABILITY; MAGNETICALLY ACTIVE STARS; MAIN-SEQUENCE EVOLUTION; DISK ACCRETION; ROTOR-PROGRAM;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Long-term homogeneous photometry for 35 classical T Tauri stars (CTTS) in the Taurus-Auriga star-forming region (SFR) has been analyzed. The original method of interstellar absorption estimation on line of sight has been proposed, taking into account the effects that are caused by magnetospheric accretion, cold spots, and extended variable circumstellar extinction. Reliable values of the interstellar extinction for 35 CTTS have been determined.
引用
收藏
页码：37 / 42
页数：6
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