Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7870
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dc.contributor.authorJadhav, Vikrant V-
dc.contributor.authorPandey, Sindhu-
dc.contributor.authorSubramaniam, A-
dc.contributor.authorSagar, R-
dc.date.accessioned2021-10-18T06:20:15Z-
dc.date.available2021-10-18T06:20:15Z-
dc.date.issued2021-10-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 42, No. 2, 89en_US
dc.identifier.issn0973-7758-
dc.identifier.urihttp://hdl.handle.net/2248/7870-
dc.descriptionRestricted Accessen_US
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractKing 2, one of the oldest clusters in the Milky Way, with an age of ∼6 Gyr and distance of ∼5700 pc, has been observed with UVIT payload on the AstroSat. With membership information derived from Gaia EDR3, the cluster is found to have 39 blue straggler stars (BSSs). We created multi-wavelength spectra-energy distributions (SED) of all the BSSs. Out of 10 UV detected BSSs, 6 bright ones were fitted with double component SEDs and were found to have hotter companions with properties similar to extreme horizontal branch (EHB)/subdwarf B (sdB) stars, with a range in luminosity and temperature, suggesting a diversity among the hot companions. We suggest that at least 15% of BSSs in this cluster are formed via mass-transfer pathway. When we compared their properties to EHBs and hotter companions to BSS in open and globular clusters, we suggest that EHB/sdBs like companions can form in binaries of open clusters as young as 6 Gyr.en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.relation.urihttps://doi.org/10.1007/s12036-021-09746-y-
dc.rights© Indian Academy of Sciences-
dc.subjectOpen star clustersen_US
dc.subjectBlue straggler starsen_US
dc.subjectExtreme horizontal branch starsen_US
dc.subjectB subdwarf starsen_US
dc.subjectUltraviolet astronomyen_US
dc.subjectSpectral energy distributionen_US
dc.subjectBinary starsen_US
dc.titleUOCS. IV. discovery of diverse hot companions to blue stragglers in the old open cluster King 2en_US
dc.typeArticleen_US
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