DISKS AROUND PRE-MAIN-SEQUENCE BINARY-SYSTEMS - THE CASE OF HARO-6-10

被引：27
|
作者：
MENARD, F
MONIN, JL
ANGELUCCI, F
ROUAN, D
机构：
[1] UNIV HEIDELBERG,INST THEORET ASTROPHYS,W-6900 HEIDELBERG 1,GERMANY
[2] OBSERV PARIS,DESPA,F-92195 MEUDON,FRANCE
来源：
ASTROPHYSICAL JOURNAL | 1993年 / 414卷 / 02期
关键词：
BINARIES; GENERAL; POLARIZATION; SCATTERING; STARS; INDIVIDUAL; (HARO-6-10); PRE-MAIN-SEQUENCE;
D O I：
10.1086/187010
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Subarcsecond KLM images of the pre-main-sequence star Haro 6-10 obtained with the CIRCUS IR camera attached to the Canada-France-Hawaii Telescope are presented. They are the first images where both components of the Haro 6-10 binary system are resolved. We confirm the results by Leinert & Haas (1989), obtained from speckle interferometry, that the projected separation of the two stars is 1.25'' at position angle 356-degrees. We also present new polarization measurement and models that suggest the presence of a flat circumbinary envelope (possibly a disk) associated with the system.
引用
收藏
页码：L117 / L120
页数：4
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