HIP 33609 b: An Eccentric Brown Dwarf Transiting a V=7.3 Rapidly Rotating B-Star
arXiv:2301.09663 · doi:10.3847/1538-3881/acd197
Abstract
We present the discovery and characterization of HIP 33609 b, a transiting warm brown dwarf orbiting a late B star, discovered by NASA's Transiting Exoplanet Survey Satellite TESS as TOI-588 b. HIP 33609 b is a large (R = 1.580 R) brown dwarf on a highly eccentric (e = 0.560) orbit with a 39-day period. The host star is a bright (V = 7.3 mag), T = 10,400 K star with a mass of M = 2.383 M and radius of R = 1.863 R, making it the hottest transiting brown dwarf host star discovered to date. We obtained radial velocity measurements from the CHIRON spectrograph confirming the companion's mass of M = 68.0 M as well as the host star's rotation rate ( km/s). We also present the discovery of a new comoving group of stars, designated as MELANGE-6, and determine that HIP 33609 is a member. We use a combination of rotation periods and isochrone models fit to the cluster members to estimate an age of 150 25 Myr. With a measured mass, radius, and age, HIP 33609 b becomes a benchmark for substellar evolutionary models.
arXiv comment16 pages, 5 figures, 4 tables, Submitted to AAS Journals
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