Field blue straggler stars: Discovery of white dwarf companions to blue metal-poor stars using UVIT/AstroSat

Abstract

Blue metal-poor (BMP) stars are the main-sequence stars that appear bluer and more luminous than normal turn-off stars of metal-poor globular clusters. They are believed to be either field blue straggler stars (FBSS) formed via post-mass transfer mechanism or accreted from dwarf satellite galaxies of the Milky Way. A significant fraction of BMP stars are discovered to be potential binaries. We observed 27 BMP stars using UVIT/\textit{AstroSat} in two FUV filters, F148W and F169M. We report the discovery of white dwarf (WD) companions of 12 BMP stars for the first time. The WD companions have estimated temperatures T${}_{eff}$ $\sim$10500 $-$ 18250 K, and masses 0.17 M${}_{\odot }$ $-$ 0.8 M${}_{\odot }$. Based on [Fe/H] and space velocity, we group the 12 BMP/FBSS stars as the thick disk (5) and halo (5), whereas two stars appear to be in-between. All the 5 thick disk BMP/FBSS have extremely low-mass (M $<$ 0.2 M${}_{\odot }$) WDs as companions, whereas the 5 halo BMP/FBSS have low (0.2 M${}_{\odot }$ $<$ M $<$ 0.4 M${}_{\odot }$), normal (0.4 M${}_{\odot }$ $<$ M $<$ 0.6M${}_{\odot }$), and high mass (M $>$ 0.6 M${}_{\odot }$) WD companions. Our analysis suggests that at least $\sim$44 $\%$ of BMP stars are FBSS, and these stars hold the key to understand the details of mass transfer, binary properties, and chemical enrichment among the FBSS.

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