MILLIMETER POLARIMETRY OF STAR-FORMING REGIONS - MAGNETIC-FIELD STRUCTURE AROUND LOW-MASS STARS

被引：0

作者：

TAMURA, M ^{[1
]}

HAYASHI, S ^{[1
]}

HOUGH, JH ^{[1
]}

机构：

[1] UNIV HERTFORDSHIRE,HATFIELD,HERTS,ENGLAND

来源：

ASTROPHYSICS AND SPACE SCIENCE | 1995年 / 224卷 / 1-2期

关键词：

INFRARED; INTERSTELLAR; CONTINUUM; POLARIZATION; STARS; FORMATION;

D O I：

10.1007/BF00667815

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have measured polarization of the 1.1 mm and 0.8 mm continuum emission for 3 pre-T Tauri stars and 2 T Tauri stars. Positive detections were made for NGC 1333 IRAS 4 and IRAS 16293-2422, while L1551 IRS 5 and HL Tau were only marginally detected. For GG Tau we measured a 2 sigma upper limit of 3%. The polarization is interpreted in terms of thermal emission by magnetically aligned dust grains in circumstellar disks or envelopes. We have found a definite geometrical relation between the polarization and other circumstellar structure.

引用

页码：21 / 24

页数：4

共 10 条

[1]

Bastien P., 1982, Astronomy & Astrophysics Supplement Series, V48, P153

[2] A SURVEY FOR CIRCUMSTELLAR DISKS AROUND YOUNG STELLAR OBJECTS [J].