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Dynamical status of Globular cluster NGC 362

Authors: Arvind K. Dattatrey, Dr. RamaKant S. Yadav;

Dynamical status of Globular cluster NGC 362

Abstract

The study of the dynamical status of the globular cluster NGC362 is presented using the spatial distribution of Blue Straggler Stars (BSSs). A significant cluster area is covered using multi-wavelength high-resolution space and ground-based data. The cluster members are selected using HST and Gaia EDR3 proper motion data sets. Using members of the cluster, the cluster’s projected density profile is created. The cluster’s radius is determined using the projected density profile. The BSS radial distribution has been used to determine the cluster’s dynamic age.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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