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New membership determination and proper motions of NGC 1817. Parametric and non-parametric approach

机译:新的成员资格确定和NGC 1817的适当议案。参数和非参数方法

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摘要

We have calculated proper motions and re-evaluated the membership probabilities of 810 stars in the area of two NGC objects, NGC 1817 and NGC 1807. We have obtained absolute proper motions from 25 plates in the reference system of the Tycho-2 Catalogue. The plates have a maximum epoch difference of 81 years; and they were taken with the double astrograph at Zo-Se station of Shanghai Observatory, which has an aperture of 40 cm and a plate scale of 30 arcsec/mm. The average proper motion precision is 1.55 mas/yr. These proper motions are used to determine the membership probabilities of stars in the region, based on there being only one very extended physical cluster: NGC 1817. With that aim, we have applied and compared parametric and non-parametric approaches to cluster/field segregation. We have obtained a list of 169 probable member stars.
机译:我们已经计算了适当的运动,并重新评估了两个NGC对象NGC 1817和NGC 1807区域中810星的隶属概率。我们从第谷2目录参考系统的25个板块中获得了绝对的正确运动。印版的最大历时差为81年;它们是在上海天文台Zo-Se站用双天文相机拍摄的,孔径为40 cm,板刻度为30 arcsec / mm。平均适当运动精度为1.55 mas / yr。这些适当的运动用于确定区域中恒星的隶属概率,因为只有一个非常扩展的物理星团:NGC1817。为此,我们已将参数和非参数方法应用于星团/场隔离。 。我们获得了169个可能的成员恒星的列表。

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