Discovery of a Planetary-mass Companion to a Brown Dwarf in Taurus
K. Todorov, K. L. Luhman, and K. K. McLeod

TL;DR
This study reports the discovery of a planetary-mass companion to a brown dwarf in Taurus, demonstrating rapid formation likely via gravitational instability, and suggests such systems can be hierarchical and form within 1 million years.
Contribution
First direct detection of a planetary-mass companion to a brown dwarf in Taurus, showing rapid formation within 1 Myr, supporting formation via gravitational instability.
Findings
Companion mass estimated at 5-10 Mjup.
Shared proper motion confirms companionship.
Possible hierarchical quadruple system.
Abstract
We have performed a survey for substellar companions to young brown dwarfs in the Taurus star-forming region using the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. In these data, we have discovered a candidate companion at a projected separation of 0.105" from one of the brown dwarfs, corresponding to 15 AU at the distance of Taurus. To determine if this object is a companion, we have obtained images of the pair at a second epoch with the adaptive optics system at Gemini Observatory. The astrometry from the Hubble and Gemini data indicates that the two objects share similar proper motions and thus are likely companions. We estimate a mass of 5-10 Mjup for the secondary based on a comparison of its bolometric luminosity to the predictions of theoretical evolutionary models. This object demonstrates that planetary-mass companions to brown dwarfs can form on a…
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