Near-infrared polarization study of L1641S
Chen, XP; Yao, YQ
刊名SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY
2005-02-01
卷号48期号:1页码:68-77
关键词near-infrared polarization star formation infrared nebula molecular outflow
ISSN号1672-1799
英文摘要H-band polarimetric images and K-S-band images of star formation region L1641S are presented. Two reflection nebulae, Re50N and Re50, are in the north and south of the region, respectively. The polarization maps of two nebulae exhibit high degrees of polarization and centrosymmetric patterns, indicating the single scattering and small dust grains in the nebulae. There are two infrared sources, IRS1 and IRS2, in the nebula Re50N. IRS1 is the illuminating source of the nebulae and the driving source of CO outflow; IRS2 is suggested to provide considerable light at optical wavelengths. The high polarization in Re50N can be interpreted as surface scattering from the outflow at an inclination of 30 degrees. Based on the polarization arc structure, we further identified the bipolar structure of the nebula Re50N. The FU Orionis phenomenon in L1641S is discussed at the end of this paper.
学科主题Physics
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Physics, Multidisciplinary
研究领域[WOS]Physics
关键词[WOS]Z-CANIS MAJORIS ; YOUNG STELLAR OBJECTS ; FU ORIONIS STARS ; IMAGING POLARIMETRY ; IRAS SOURCES ; REIPURTH 50 ; RNO 1B/1C ; REGION ; (CO)-C-13 ; SPECTRUM
收录类别SCI
语种英语
WOS记录号WOS:000228224000007
公开日期2012-03-07
内容类型期刊论文
源URL[http://159.226.72.40/handle/332002/4076]  
专题紫金山天文台_毫米波和亚毫米波技术实验室
作者单位Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
推荐引用方式
GB/T 7714
Chen, XP,Yao, YQ. Near-infrared polarization study of L1641S[J]. SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY,2005,48(1):68-77.
APA Chen, XP,&Yao, YQ.(2005).Near-infrared polarization study of L1641S.SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY,48(1),68-77.
MLA Chen, XP,et al."Near-infrared polarization study of L1641S".SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY 48.1(2005):68-77.
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