Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7494
Title: Radial distribution of Blue Stragglers in NGC 5466 using AstroSat
Authors: Snehalata Sahu
Subramaniam, A
Keywords: Galaxy:globular clusters: individual (NGC 5466)
stars: Blue Stragglers
stars: horizontal-branch
ultraviolet: stars
Issue Date: May-2019
Publisher: Cambridge University Press
Citation: Proceedings of the International Astronomical Union, Vol. 351 , pp. 498-501
Series/Report no.: IAU Symposium No. 351;
Abstract: We present the results obtained from Near-UV observations of the cluster NGC 5466 taken with UVIT onboard AstroSat to study the radial distribution of Blue Straggler Stars (BSSs), covering the cluster region up to a radius of 14'. Our study confirms that the BSSs are more centrally concentrated than Horizontal Branch (HB) stars in the cluster. We do not find a statistically significant rising trend in the radial distribution of BSSs for the outer regions, as most of the previously catalogued BSSs that are located in the cluster outskirts were found to be non-members, quasars or galaxies. This study highlights the importance of UV imaging combined with membership information to probe the radial distribution of BSSs.
Description: Restricted Access © International Astronomical Union https://doi.org/10.1017/S1743921319006835
URI: http://prints.iiap.res.in/handle/2248/7494
ISSN: 1743-9213
Appears in Collections:IIAP Publications

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