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首页> 外文期刊>Astronomy and astrophysics >Polarimetric survey of main-belt asteroids - IV. New results from the first epoch of the CASLEO survey
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Polarimetric survey of main-belt asteroids - IV. New results from the first epoch of the CASLEO survey

机译:主带小行星的极化测量-IV。 CASLEO调查第一个时期的新结果

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Aims. We present results of a polarimetric survey of main-belt asteroids at Complejo Astronómico El Leoncito (CASLEO), San Juan, Argentina. The aims of this survey are to increase the database of asteroid polarimetry, to estimate diversity in polarimetric properties of asteroids that belong to different taxonomic classes, and to search for objects that exhibit anomalous polarimetric properties. Methods. The data were obtained using the Torino and CASPROF polarimeters at the 2.15m telescope. The Torino polarimeter is an instrument that allows simultaneous measurement of polarization in five different bands, and the CASPROF polarimeter is a two-hole aperture polarimeter with rapid modulation. Results. The survey began in 1995, and until 2012 data on a large sample of asteroids were obtained. We here present and analyze the unpublished results for 129 asteroids of different taxonomic types, 56 which were polarimetrically observed for the first time. We find that the asteroids (402) Chloe and (729) Watsonia are Barbarians, and asteroid (269) Justitia shows a phase – polarization curve that seems to have a small inversion angle. Data obtained in UBVRI colors allow us to sketch an analysis of the wavelength dependence of the degree of linear polarization for 31 asteroids, in spite of some large error bars in some cases.
机译:目的我们介绍了在阿根廷圣胡安市ComplejoAstronómicoEl Leoncito(CASLEO)进行的主带小行星的极化测量结果。这项调查的目的是增加小行星极化的数据库,估计属于不同分类学类别的小行星的极化特性的多样性,并搜索表现出异常极化特性的物体。方法。数据是使用2.15m望远镜上的Torino和CASPROF旋光仪获得的。都灵(Torino)旋光仪是一种可以同时测量五个不同波段的偏振光的仪器,而CASPROF旋光仪是具有快速调制功能的两孔孔径旋光仪。结果。该调查始于1995年,直到2012年,才获得了大量小行星样本的数据。我们在这里展示并分析了129种不同分类类型的小行星的未发表结果,其中56种是首次用极化技术观察到的。我们发现小行星(402)克洛伊(Chloe)和(729)瓦托尼亚(Watsonia)是蛮族,而小行星(269)Justitia则显示出相位-极化曲线,其反角似乎很小。尽管在某些情况下存在一些较大的误差线,但通过UBVRI颜色获得的数据使我们能够对31个小行星的线性偏振度的波长依赖性进行分析。

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