# UVIT Open Cluster Study. I. Detection of a White Dwarf Companion to a Blue Straggler in M67: Evidence of Formation through Mass Transfer

## TL;DR

This study reports the first direct detection of a white dwarf companion to a blue straggler star in M67, providing evidence that such stars can form through mass transfer in binary systems.

## Contribution

The paper presents the first direct detection of a white dwarf companion to a blue straggler in M67, supporting the mass transfer formation pathway.

## Key findings

- White dwarf companion detected around WOCS1007 in M67.
- The companion has a temperature of 13250-13750K and a low mass (~0.18 M_sun).
- WOCS1007 likely formed via mass transfer in a close binary system.

## Abstract

The old open cluster M67, populated with blue straggler stars (BSSs), is a well known test bed to study the BSS formation pathways. Here, we report the first direct detection of a white dwarf (WD) companion to a BSS in M67, using far-UV images from the \textit{Ultra Violet Imaging telescope} ({\it UVIT}) on {\it ASTROSAT}. Near-simultaneous observations in three far-UV bands combined with {\it GALEX}, {\it IUE}, ground and space based photometric data covering 0.14 -11.5 $\mu$m range for WOCS1007 were found to require a binary fit to its spectral energy distribution (SED), consisting of a BSS and a hot companion. On the other hand, a single spectral fit was found to be satisfactory for the SEDs of two other BSSs, WOCS1006 and WOCS2011, with the latter showing a deficient far-UV flux. The hot companion of WOCS1007 is found to have a T$_{eff}$ $\sim$ 13250-13750K and a radius of 0.09$\pm$0.01 R$_\odot$. A comparison with WD models suggests it to be a low mass WD ($\sim$ 0.18$M_\odot$), in agreement with the kinematic mass from the literature. As a low mass WD ($<$ 0.4$M_\odot$) necessitates formation through mass transfer (MT) in close binaries, WOCS1007 with a known period of 4.2 days along with its fast rotation, is likely to be formed by a case A or case B binary evolution.