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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/handle/123456789/14213
Title: Tidal tails in the disintegrating open cluster NGC 752
Authors: Vaidya, Kaushar
Keywords: Physics
Methods: data analysis
Open clusters and associations: individual: NGC 752
Issue Date: Aug-2021
Publisher: OUP
Abstract: We utilize the robust membership determination algorithm, ML-MOC, on the precise astrometric and deep photometric data from Gaia Early Data Release 3 within a region of radius 5° around the centre of the intermediate-age Galactic open cluster NGC 752 to identify its member stars. We report the discovery of the tidal tails of NGC 752, extending out to ∼35 pc on either side of its denser central region and following the cluster orbit. From comparison with PARSEC stellar isochrones, we obtain the mass function of the cluster with a slope, χ = −1.26 ± 0.07. The high negative value of χ is indicative of a disintegrating cluster undergoing mass segregation. χ is more negative in the intra-tidal regions as compared to the outskirts of NGC 752. We estimate a present day mass of the cluster, M⊙. Through mass-loss due to stellar evolution and tidal interactions, we further estimate that NGC 752 has lost nearly 95.2–98.5 per cent of its initial mass, Mi = 0.64–2 × 104 M⊙.
URI: https://academic.oup.com/mnras/article/505/2/1607/6276753
http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14213
Appears in Collections:Department of Physics

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