The Companions to B and A Stars Snapshot (C-BASS) Survey: I. Discovery of a Young Brown Dwarf Companion to HIP 17453
Marah Brinjikji, Adam J. Smith, Jennifer Patience, Eric Nielsen, Austin Ware, Jorge A. Sanchez, Robert J. De Rosa, Jasmine Garani, Emma Softich, Michael C. Liu, Bruce Macintosh, Thomas M. Esposito, Brendan P. Bowler, William M. Best, Sarah Blunt, Trent Dupuy, Justin Hom, Jessica A. Klusmeyer, Franck Marchis, Jayke S. Nguyen, Anne E. Peck, Mark W. Phillips, William Roberson, Jean-Baptiste Ruffio, William Thompson, Zahed Wahhaj, Samuel A. Walker, Jason J. Wang, Patrick A. Young
astro-ph.SR, astro-ph.EP
Submitted: 2026-06-29
Comments: 30 pages, 15 figures, 4 tables, accepted in the Astronomical Journal
License: http://creativecommons.org/licenses/by/4.0/
The gist: We report the detection of a new brown dwarf companion to HIP 17453 A, a chemically peculiar A0V star located at a distance of 81 pc.
Terminology
Abstract
We report the detection of a new brown dwarf companion to HIP 17453 A, a chemically peculiar A0V star located at a distance of 81 pc. HIP 17453 A was observed with high-resolution adaptive optics imaging using the Near-Infrared Camera 2 on the Keck II telescope as part of the Companions to B and A Stars Snapshot (C-BASS) survey over a ten-year baseline, revealing the presence of a companion with proper motion consistent with the primary. We estimate the age of the HIP 17453 system as 280 plus or minus 125 Myr, and with follow-up intermediate resolution (R 1800) spectroscopic observations with the Gemini Near Infra-Red Spectrograph (GNIRS) on the Gemini-North telescope, we found the spectrum of HIP 17453 B to be consistent with a spectral type of L2 plus or minus 1. Through interpolation of Sonora Diamondback evolutionary models, we calculate an effective temperature of 1953+84-78 K and mass of 53+10-8 M Jup for HIP 17453 B, which corresponds to a mass ratio of q = 0.024 plus or minus 0.004 for the HIP 17453 system. With its intermediate mass and young age, HIP 17453 B joins a small set of benchmark brown dwarf companions around early-type stars that are suitable for follow-up atmospheric and evolutionary studies.
Sources
- The SpeX Prism Library Analysis Toolkit (SPLAT): A Data Curation Model
- Planet Formation Theory in the Era of ALMA and Kepler: from Pebbles to Exoplanets
- Modernizing IRAF to Support Gemini Data Reduction
- The high-contrast performance of the Keck Planet Imager and Characterizer
- Brown Dwarf Formation: Theory
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