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The astrophysical behavior of open clusters along the Milky Way Galaxy

机译:银河系周围开放星团的天体行为

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The main aim of this paper is to study the astrophysical behaviour of open clusters’ properties along the Milky Way Galaxy. Near-IRJHKS(2MASS) photometry has been used for getting a homogeneous Catalog of 263 open clusters’ parameters, which are randomly selected and studied by the author through the last five years; most of them were studied for the first time. The correlations between the astrophysical parameters of these clusters have been achieved by morphological way and compared with the most recent works.
机译:本文的主要目的是研究银河系周围开放星团性质的天体行为。最近IRJHKS(2MASS)光度法已被用于获得263个开放星团参数的均匀目录,作者在最近五年中对其进行了随机选择和研究。他们中的大多数是第一次学习。这些星团的天体物理参数之间的相关性已经通过形态学的方法得以实现,并与最新的工作进行了比较。

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