首页> 外文期刊>The Astrophysical Journal. Letters >NEAR-INFRARED CIRCULAR POLARIZATION SURVEY IN STAR-FORMING REGIONS: CORRELATIONS AND TRENDS
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NEAR-INFRARED CIRCULAR POLARIZATION SURVEY IN STAR-FORMING REGIONS: CORRELATIONS AND TRENDS

机译:恒星形成区域的近红外圆极化调查:相关性和趋势

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摘要

We have conducted a systematic near-infrared circular polarization (CP) survey in star-forming regions, covering high-mass, intermediate-mass, and low-mass young stellar objects. All the observations were made using the SIRPOL imaging polarimeter on the Infrared Survey Facility 1.4 m telescope at the South African Astronomical Observatory. We present the polarization properties of 10 sub-regions in 6 star-forming regions. The polarization patterns, extents, and maximum degrees of linear and circular polarizations are used to determine the prevalence and origin of CP in the star-forming regions. Our results show that the CP pattern is quadrupolar in general, the CP regions are extensive, up to 0.65 pc, the CP degrees are high, up to 20%, and the CP degrees decrease systematically from high- to low-mass young stellar objects. The results are consistent with dichroic extinction mechanisms generating the high degrees of CP in star-forming regions.
机译:我们在恒星形成区域进行了系统的近红外圆极化(CP)调查,涵盖高质量,中质量和低质量的年轻恒星物体。所有的观察都是使用SIRPOL成像旋光仪在南非天文台1.4 m红外勘测设备上进行的。我们介绍了6个恒星形成区域中10个子区域的偏振特性。线偏振和圆偏振的偏振模式,程度以及最大程度用于确定恒星形成区域中CP的发生率和起源。我们的结果表明,CP模式总体上是四极的,CP区域广泛,高达0.65 pc,CP度高,高达20%,并且CP度从高质量的低质量的年轻恒星物体系统地降低。 。该结果与在恒星形成区域产生高度CP的二向色性消光机制一致。

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