2MASS 0213+3648 C: A wide T3 benchmark companion to an an active, old M dwarf binary
Authors:
Deacon et al
Abstract:
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+6.4−4.0 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 Hα emission and shows evidence for UV flares. The binary's weak {\it GALEX} UV emission and strong Na I 8200\AA Na absorption leads us to an age range of ∼1-10Gyr. Applying this age range to evolutionary models implies the wide companion has a mass of 0.063±0.009\,M⊙. 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.
Friday, September 15, 2017
2MASS 0213+3648 C: A wide T3 benchmark companion to an an active, old M dwarf binary
Labels:
2MASS 0213+3648C,
brown dwarf,
multi stellar systems,
T class,
T Dwarf
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