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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7500
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dc.contributor.authorKumar, R-
dc.contributor.authorPradhan, A. C-
dc.contributor.authorParthasarathy, M-
dc.contributor.authorOjha, D. K-
dc.contributor.authorMohapatra, A-
dc.contributor.authorMurthy, J-
dc.date.accessioned2020-11-27T12:53:31Z-
dc.date.available2020-11-27T12:53:31Z-
dc.date.issued2019-05-
dc.identifier.citationProceedings of the International Astronomical Union, Vol. 351, pp. 464-467en_US
dc.identifier.issn1743-9213-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7500-
dc.descriptionRestricted Access © International Astronomical Union https://doi.org/10.1017/S1743921319007373en_US
dc.description.abstractWe have performed photometric analysis of four Galactic globular clusters (GGCs): NGC 4147, NGC 4590, NGC 5053 and NGC 7492 using far-UV and near-UV filters of the Ultraviolet Imaging Telescope (UVIT) on-board AstroSat. With the help of color-magnitude diagrams (CMDs), we have identified ~150 blue horizontal branch stars (BHBs), and ~40 blue straggler stars (BSS) in the four GGCs. We study the temperature and radial distribution of BHBs and BSS for the four GGCs.en_US
dc.language.isoenen_US
dc.publisherCambridge University Pressen_US
dc.relation.ispartofseriesIAU Symposium No. 351;-
dc.subjectglobular clusters: individual (NGC 4147, NGC 4590, NGC 5053 and NGC 7492)en_US
dc.subjectstars: horizontal-branchen_US
dc.subjecttechniques: photometricen_US
dc.titleUVIT observations of UV-Bright stars in four Galactic Globular Clustersen_US
dc.typeArticleen_US
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