{ "id": "1908.01573", "version": "v1", "published": "2019-08-05T12:05:17.000Z", "updated": "2019-08-05T12:05:17.000Z", "title": "Detection of White Dwarf Companions to Blue Straggler Stars from UVIT Observations of M67", "authors": [ "Sindhu N", "Annapurni Subramaniam", "Aaron M Geller", "Vikrant Jadhav", "Christian Knigge", "Mirko Simunovic", "Nathan Leigh", "Michael Shara", "Thomas H Puzia" ], "comment": "4 pages, 2 figures, to appear in IAU Symposium No. 351 proceedings - Star Clusters: From the Milky Way to the Early Universe, 2019", "categories": [ "astro-ph.SR", "astro-ph.GA" ], "abstract": "We investigate the old open cluster M67 using ultraviolet photometric data of Ultra-Violet Imaging Telescope in multi-filter far-UV bands. M67, well known for the presence of several blue straggler stars (BSS), has been put to detailed tests to understand their formation pathways. Currently, there are three accepted formation channels: mass transfer due to Roche-lobe overflow in binary systems, stellar mergers either due to dynamical collisions or through coalescence of close binaries. So far, there had not been any confirmed detection of a white dwarf (WD) companion to any of the BSSs in this cluster. Here, we present the detection of WD companions to 5 bright BSSs in M67. The multiwavelength spectral energy distributions covering 0.12 -11.5 $\\mu$m range, were found to require binary spectral fits for 5 BSSs, consisting of a cool (BSS) and a hot companion. The parameters (Luminosity, Temperature, Radius and Mass) of the hot companions suggest them to be WDs with mass in the range 0.2 - 0.35 M$_{\\odot}$ with T$_{eff}$ $\\sim$ 11000 - 24000 K.", "revisions": [ { "version": "v1", "updated": "2019-08-05T12:05:17.000Z" } ], "analyses": { "keywords": [ "blue straggler stars", "white dwarf companions", "uvit observations", "spectral energy distributions covering", "hot companion" ], "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable" } } }