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We present the discovery of a 360 AU separation T3 companion to the tight (3.1 AU) M4.5+M6.5 binary 2MASS J02132062+3648506. This companion was identified using Pan-STARRS1 data and, despite its relative proximity to the Sun (22.2$_{-4.0}^{+6.4}$ pc; Pan-STARRS1 parallax) and brightness ($J$=15.3), appears to have been missed by previous studies due to its position near a diffraction spike in 2MASS. The close M~dwarf binary has active X-ray and H$alpha$ emission and shows evidence for UV flares. The binarys weak {it GALEX} UV emission and strong Na I 8200AA Na absorption leads us to an age range of $sim$1-10Gyr. Applying this age range to evolutionary models implies the wide companion has a mass of 0.063$pm$0.009,$M_{odot}$. 2MASS J0213+3648 C provides a relatively old benchmark close to the L/T transition and acts as a key, older comparison to the much younger early-T companions HN~Peg~B and GU~Psc~b.
Low-mass and brown dwarfs have recently been found as wide companions to many nearby stars, formerly believed to be single. Wide binaries are usually found as common proper motion pairs. Sometimes, more than two objects share the same large proper mo
We present the discovery of only the third brown dwarf known to eclipse a non-accreting white dwarf. Gaia parallax information and multi-colour photometry confirm that the white dwarf is cool (9950$pm$150K) and has a low mass (0.45$pm$0.05~MSun), and
PSR,J1723$-$2837 is a redback millisecond pulsar (MSP) with a low-mass companion in a 14.8,h orbit. The systems properties closely resemble those of transitional MSPs that alternate between spin-down and accretion-powered states. In this paper we rep
Asteroseismology of bright stars has become increasingly important as a method to determine fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiated a revolution by detecting oscillations in more than 500 main-sequen
We present the discovery of CWISE J203546.35-493611.0, a peculiar M8 companion to the M4.5 star APMPM J2036-4936 discovered through the citizen science project Backyard Worlds: Planet 9. Given CWISE J203546.35-493611.0s proper motion ($mu_{alpha}$, $