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Study of open cluster NGC 5617 in Gaia era

Published online by Cambridge University Press:  14 May 2020

D. Bisht
Affiliation:
Key Laboratory for Researches in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui, 230026
Qingfeng Zhu
Affiliation:
Key Laboratory for Researches in Galaxies and Cosmology, University of Science and Technology of China, Chinese Academy of Sciences, Hefei, Anhui, 230026
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Abstract

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Identification of member stars in open clusters is still an open question. Thanks to Gaia DR2 data base, which improves our statistics regarding true members in clusters to understand cluster properties much better way. In this paper, we identify the cluster members using proper motion and colour magnitude diagram for NGC 5617. In addition to this, we have determined more precise fundamental parameters as well.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020

References

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