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Study of open cluster NGC 5617 in Gaia era

Published online by Cambridge University Press:  14 May 2020

D. Bisht Open the ORCID record for D. Bisht [Opens in a new window]  and
Qingfeng Zhu
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.

Keywords

Open clusters and associations: individual (NGC 5617)Colour-magnitude diagramAstrometry
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S353: Galactic Dynamics in the Era of Large Surveys , June 2019 , pp. 22 - 23
Copyright
© International Astronomical Union 2020

References

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