2MASS J18450079–1409036 and 2MASS J18450097–1409053 is a system of two red dwarf stars both of which have spectral types of M5,[6] with projected separation of 3.2 seconds of arc.
The Gaia parallaxes place the system at 18.2 parsecs (59 light-years) from Earth.
[1][3] Kinematically, it belongs to young (30-50 million years) Argus association.
[2] 2MASS J18450079–1409036 and 2MASS J18450097-1409053 appear to be a common proper motion pair,[8] confirmed to be bound in 2016.
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