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Distance moduli of open cluster NGC 6819 from Red Giant Clump stars

机译:疏散星团NGC 6819与红巨星团星的距离模

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In this paper we study Kepler open cluster NGC 6819 using Kepler data of Red Giant Clump (RGC) single member (SM) stars. The Kepler data spans a period of 4 years starting in 2009. In particular, we derive distance moduli for each individual RGC star, from which we get the mean distance modulus of mu(0) = 11.520 +/- 0.105 mag for the cluster when we use reddening from the Kepler Input Catalogue (KIC) for each RGC star. A value of mu(0) = 11.747 +/- 0.086 mag is obtained when uniform reddening value E(B - V) = 0.15 is used for the cluster. The values of go obtained with RGC stars are in agreement with the values in the literature with other methods. We report for the case of Kepler open cluster NGC 6819 that RGC stars can be used as 'distance candles' as has been done in the literature with other open clusters. (C) 2016 Elsevier B.V. All rights reserved.
机译:在本文中,我们使用红巨团(RGC)单员(SM)星的开普勒数据研究开普勒开星团NGC 6819。开普勒数据从2009年开始为期4年。特别是,我们推导出每个RGC恒星的距离模量,从中我们得出该星团的平均距离模量mu(0)= 11.520 +/- 0.105 mag我们对每个RGC星使用开普勒输入目录(KIC)的变红。当对簇使用统一的变红值E(B-V)= 0.15时,将获得mu(0)= 11.747 +/- 0.086 mag的值。用RGC恒星获得的go值与文献中其他方法的值一致。对于开普勒开放星团NGC 6819,我们报告说RGC恒星可以用作“远距离蜡烛”,正如其他开放星团在文献中所做的那样。 (C)2016 Elsevier B.V.保留所有权利。

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