K'-band polarimetric imaging of S187IR and S233

CORC > 紫金山天文台 > 中国科学院紫金山天文台 > 分子云与恒星形成研究团组

	K'-band polarimetric imaging of S187IR and S233
	Jiang, ZB; Yao, YQ ; Yang, J; Ishii, M ; Nagata, T ; Nakaya, H ; Sato, S
刊名	ASTRONOMICAL JOURNAL
	2001-07-01
卷号	122 期号:1 页码:313-321
关键词	infrared radiation ISM : individual (S187, S233) ISM : lines and bands polarization reflection nebulae stars : formation
英文摘要	K'-band polarimetric images of star-forming regions S187 IR and S233 are presented. In S187 IR, a bipolar, near-infrared nebula is observed around IRAS 01202+6133, with the southern part being bright and knotty, and the northern part being faint and filamentary. The polarization pattern shows that the nebula is illuminated by a single near-infrared source, which is associated with IRAS 01202+6133. A polarization disk is found around this source with the disk plane roughly perpendicular to the axis of the bipolar nebula. We conclude that this source is the driving source of the outflow in the region. Two nebulae are detected in the S233 region. Associated with a compact infrared cluster, S233 A is roughly round in shape and shows a weak polarization pattern. The S233 B nebula shows roughly elongated geometry in the east-west direction. The polarization vectors divide it into three parts. Each part has distinctly different polarization from the others. The northeastern part of S233 B exhibits a centrosymmetric polarization pattern around a centroid, at which we locate a deeply embedded source (DES) undetected in the K' band and shorter wavelengths. The DES is likely the exciting source of water masers and outflows in the S233 B region. The western part of the nebula shows a parallel polarization pattern, but the southeastern part displays very little polarization. Comparison of the morphology and polarization of the nebulae in different star-forming regions suggests a close relationship between the evolutionary sequence of the young stellar objects and the morphology of the associated nebulae.
WOS标题词	Science & Technology ; Physical Sciences
类目[WOS]	Astronomy & Astrophysics
研究领域[WOS]	Astronomy & Astrophysics
关键词[WOS]	YOUNG STELLAR OBJECTS ; MOLECULAR OUTFLOW SOURCES ; STAR-FORMING REGIONS ; IRAS POINT SOURCES ; H-II REGIONS ; POLARIZATION MAPS ; INFRARED SOURCES ; BIPOLAR NEBULAE ; HII-REGIONS ; IRS
收录类别	SCI
语种	英语
WOS记录号	WOS:000169943300026
内容类型	期刊论文
源URL	[http://libir.pmo.ac.cn/handle/332002/15793]
专题	紫金山天文台_分子云与恒星形成研究团组
作者单位	1.Chinese Acad Sci, Natl Astron Observ, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China 2.Nagoya Univ, Fac Sci, Dept Astrophys, Nagoya, Aichi 4648602, Japan
推荐引用方式 GB/T 7714	Jiang, ZB,Yao, YQ,Yang, J,et al. K'-band polarimetric imaging of S187IR and S233[J]. ASTRONOMICAL JOURNAL,2001,122(1):313-321.
APA	Jiang, ZB.,Yao, YQ.,Yang, J.,Ishii, M.,Nagata, T.,...&Sato, S.(2001).K'-band polarimetric imaging of S187IR and S233.ASTRONOMICAL JOURNAL,122(1),313-321.
MLA	Jiang, ZB,et al."K'-band polarimetric imaging of S187IR and S233".ASTRONOMICAL JOURNAL 122.1(2001):313-321.