Searching for GEMS: Discovery of the Nearby Post-Common-Envelope Binary System TIC-460388167

Abstract

Short-period white dwarf+main-sequence binaries are Post-Common-Envelope Binaries (PCEB) that have survived a common envelope phase. Such systems, if detached and eclipsing, enable precise measurements of the constituent stars, providing a unique opportunity to probe the effects of the common envelope phase on the system. We report the discovery of one such nearby (57 pc) system, TIC-460388167, using a combination of multi-band photometric light curves and spectroscopic radial velocities. In addition to eclipses, the system exhibits a continuously variable light curve that we model as a combination of ellipsoidal variations and star spots. We determine a period $P$=0.63596258$\pm$0.00000012 d and inclination $i$=89.0$\pm$0.4 deg. The best-fitting model specifies a white dwarf with T${}_1$=7607$\pm$127 K and radius R${}_1$=0.0131$\pm$0.0003 $R_{\odot }$, which is eclipsed by a T${}_2$=3151 $\pm$ 59 K, R${}_2$=0.327$\pm$0.006 $R_{\odot }$ M dwarf. The white dwarf mass is 0.61$\pm$0.04 M${}_{\odot }$. We present the first velocity resolved profile for a PCEB secondary and show that the rotation of the M-dwarf is synchronous with the orbital period, as expected. We compare the constituent stars to other PCEB systems and find TIC-460388167A is one of the coolest known white dwarfs in such systems. TIC-460388167 is among the longest period eclipsing PCEB systems known.