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Title: Verification of Gaia Data Release 3 Single-lined Spectroscopic Binary Solutions With Three Transiting Low-mass Secondaries
Abstract

While secondary mass inferences based on single-lined spectroscopic binary (SB1) solutions are subject tosinidegeneracies, this degeneracy can be lifted through the observations of eclipses. We combine the subset of Gaia Data Release 3 SB1 solutions consistent with brown dwarf-mass secondaries with the Transiting Exoplanet Survey Satellite (TESS) Object of Interest (TOI) list to identify three candidate transiting brown dwarf systems. Ground-based precision radial velocity follow-up observations confirm that TOI-2533.01 is a transiting brown dwarf withM=723+3MJup=0.0690.003+0.003Morbiting TYC 2010-124-1 and that TOI-5427.01 is a transiting very low-mass star withM=932+2MJup=0.0880.002+0.002Morbiting UCAC4 515-012898. We validate TOI-1712.01 as a very low-mass star withM=827+7MJup=0.0790.007+0.007Mtransiting the primary in the hierarchical triple system BD+45 1593. Even after accounting for third light, TOI-1712.01 has a radius nearly a factor of 2 larger than predicted for isolated stars with similar properties. We propose that the intense instellation experienced by TOI-1712.01 diminishes the temperature gradient near its surface, suppresses convection, and leads to its inflated radius. Our analyses verify Gaia DR3 SB1 solutions in the low Doppler semiamplitude limit, thereby providing the foundation for future joint analyses of Gaia radial velocities and Kepler, K2, TESS, and PLAnetary Transits and Oscillations light curves for the characterization of transiting massive brown dwarfs and very low-mass stars.

 
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NSF-PAR ID:
10472903
Author(s) / Creator(s):
; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more » ; « less
Publisher / Repository:
DOI PREFIX: 10.3847
Date Published:
Journal Name:
The Astronomical Journal
Volume:
166
Issue:
6
ISSN:
0004-6256
Format(s):
Medium: X Size: Article No. 225
Size(s):
["Article No. 225"]
Sponsoring Org:
National Science Foundation
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