EQ Pegasi
EQ Pegasi is a nearby binary system of two red dwarfs. Both components are flare stars, with spectral types of M4Ve and M6Ve respectively, and a current separation between the components of 5.8 arcseconds. The system is at a distance of 20.4 light-years, and is 950 million years old. The primary star is orbited by one known exoplanet.
Discovery
EQ Pegasi was first noticed to be a binary star by Carl A. Wirtanen who in the course of a systematic survey of the McCormick Observatory photographic plates for M-type dwarfs, detected a companion about two magnitudes fainter at a separation of 3.5 arcseconds.Both components were also thought to be single-lined spectroscopic binaries, with faint companions that have not been resolved in orbits of a few years, but this is no longer thought to be the case. A 2021 study of nearby stars states that "the spectroscopic binarity classification is almost certainly due to activity".