Abstract
We present the discovery of NGTS-7Ab, a high mass brown dwarf transiting
an M dwarf with a period of 16.2 hours, discovered as part of the Next
Generation Transit Survey (NGTS). This is the shortest period transiting
brown dwarf around a main or pre-main sequence star to date. The M star
host (NGTS-7A) has an age of roughly 55 Myr and is in a state of
spin-orbit synchronisation, which we attribute to tidal interaction with
the brown dwarf acting to spin up the star. The host star is
magnetically active and shows multiple flares across the NGTS and follow
up lightcurves, which we use to probe the flare-starspot phase relation.
The host star also has an M star companion at a separation of 1.13
arcseconds with very similar proper motion and systemic velocity,
suggesting the NGTS-7 system is a hierarchical triple. The combination
of tidal synchronisation and magnetic braking is expected to drive
ongoing decay of the brown dwarf orbit, with a remaining lifetime of
only 5-10 Myr.
| Original language | English |
|---|---|
| Journal | Monthly Notices of the Royal Astronomical Society, Advance Access |
| DOIs | |
| Publication status | Published - 11 Sept 2019 |
Keywords
- stars: brown dwarfs
- stars: low mass
- stars: rotation
- stars: individual: NGTS-7A
- stars: flare
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Dive into the research topics of 'NGTS-7Ab: An ultra-short period brown dwarf transiting a tidally-locked and active M dwarf'. Together they form a unique fingerprint.Student theses
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Understand thy star, understand thy planet
Costes, J. (Author), Watson, C. (Supervisor) & de Mooij, E. (Supervisor), Dec 2021Student thesis: Doctoral Thesis › Doctor of Philosophy
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