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Using data from the MEarth-North and MEarth-South transit surveys, we presentthe detection of eclipses in four mid M-dwarf systems: LP 107-25, LP 261-75, LP796-24, and LP 991-15. Combining the MEarth photometry with spectroscopicfollow-up observations, we show that LP 107-25 and LP 796-24 are short-period(1.388 and 0.523 day, respectively) eclipsing binaries in triple-lined systemswith substantial third light contamination from distant companions. LP 261-75is a short-period (1.882 day) single-lined system consisting of a mid M-dwarfeclipsed by a probable brown dwarf secondary, with another distant visual browndwarf companion. LP 991-15 is a long-period (29.3 day) double-lined eclipsingbinary on an eccentric orbit with a geometry which produces only primaryeclipses. A spectroscopic orbit is given for LP 991-15, and initial orbits forLP 107-25 and LP 261-75.

Four new eclipsing mid M-dwarf systems from the New Luyten Two Tenths catalog