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Please use this identifier to cite or link to this item: http://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14214
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dc.contributor.authorVaidya, Kaushar-
dc.date.accessioned2024-02-12T06:50:10Z-
dc.date.available2024-02-12T06:50:10Z-
dc.date.issued2019-
dc.identifier.urihttps://www.aanda.org/articles/aa/abs/2019/04/aa34449-18/aa34449-18.html-
dc.identifier.urihttp://dspace.bits-pilani.ac.in:8080/jspui/xmlui/handle/123456789/14214-
dc.description.abstractBlue straggler stars (BSSs) are observed in Galactic globular clusters and old open clusters. The radial distribution of BSSs has been used to diagnose the dynamical evolution of globular clusters. For the first time, with a reliable sample of BSSs identified with Gaia DR2, we conduct such an analysis for an open cluster.en_US
dc.language.isoenen_US
dc.publisherThe European Southern Observatoryen_US
dc.subjectPhysicsen_US
dc.subjectBlue stragglers / open clusters and associationsen_US
dc.subjectBerkeley 17 / methodsen_US
dc.subjectData analysisen_US
dc.titleThe blue straggler population of the old open cluster Berkeley 17en_US
dc.typeArticleen_US
Appears in Collections:Department of Physics

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