Cited by 207Stellar, planetary, and galactic studiesAstrophysics and Star Formation StudiesAstronomy and Astrophysical Research

Mapping the Shores of the Brown Dwarf Desert. I. Upper Scorpius

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Kraus, Adam L., Ireland, Michael J., Martinache, Frantz, Lloyd, James P.·2008·The Astrophysical Journal

Abstract

We present the results of a survey for stellar and substellar companions to 82 young stars in the nearby OB association Upper Scorpius. This survey used nonredundant aperture mask interferometry to achieve typical contrast limits of Δ K ∼ 5–6 at the diffraction limit, revealing 12 new binary companions that lay below the detection limits of traditional high-resolution imaging; we also summarize a complementary snapshot imaging survey that discovered seven directly resolved companions. The overall frequency of binary companions (~35 −4 +5 % at separations of 6-435 AU) appears to be equivalent to field stars of similar mass, but companions could be more common among lower mass stars than for the field. The companion mass function has statistically significant differences compared to several suggested mass functions for the field, and we suggest an alternate lognormal parameterization of the mass function. Our survey limits encompass the entire brown dwarf mass range, but we only detected a single companion that might be a brown dwarf; this deficit resembles the so-called brown dwarf desert that has been observed by radial velocity planet searches. Finally, our survey's deep detection limits extend into the top of the planetary mass function, reaching 8-12 M Jup for half of our sample. We have not identified any planetary companions at high confidence (≳99.5%), but we have identified four candidate companions at lower confidence (≳97.5%) that merit additional follow-up to confirm or disprove their existence.

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Research works printed but not linked: 8

  1. Cameron, P. B. 2008, Ph.D. thesis, Caltech Chabrier, G., et al. 2000, ApJ, 542, 464
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Authors
Kraus, A. L., Ireland, M. J., Martinache, F., & Lloyd, J. P.
Affiliations
  • California Institute of Technology (US)
  • Cornell University (US)
Venue
The Astrophysical Journal
Published
2008-05-20
Volume
679
Issue
1
Pages
762-782
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2028041709
Cited by
207
References
82
Citations by year
2026: 3 · 2025: 2 · 2023: 6 · 2022: 11 · 2021: 5 · 2020: 13 · 2019: 23 · 2018: 20 · 2017: 10 · 2016: 25 · 2015: 12 · 2014: 12 · 2013: 12 · 2012: 19
FWCI
6.61
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • ANU Open Research (Australian National University) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (0506588, 0705085)
  • National Aeronautics and Space Administration
  • California Institute of Technology
  • U.S. Naval Observatory
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
  • Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
Keywords
brown dwarf desert, brown dwarfs, Upper Scorpius, OB associations, binary companion, substellar companions, stellar multiplicity, young stars

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