Cited by 153Stellar, planetary, and galactic studiesAstrophysics and Star Formation StudiesGalaxies: Formation, Evolution, Phenomena

Statistical properties of brown dwarf companions: implications for different formation mechanisms

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Ma, Bo, Ge, Jian·2014·Monthly Notices of the Royal Astronomical Society

Abstract

The mass domain where massive extrasolar planets and brown dwarfs overlap is still poorly understood due to the paucity of brown dwarfs orbiting close to solar-type stars, the so-called brown dwarf desert. In this paper, we collect all available data about close brown dwarfs around solar-type stars and their host stars from literature and study the demographics of the brown dwarf desert. The data clearly show a short period and a medium mass gap in the brown dwarf period–mass distribution diagram (35 < m sin i < 55MJup and P < 100 d), representing the ‘driest land’ in the brown dwarf desert. Observation biases are highly unlikely to cause this gap due to its short period and medium mass, of which brown dwarfs can be easily detected by previous radial velocity surveys. Brown dwarfs above and below this gap have significantly different eccentricity distribution, which not only confirms that this gap is real, but also implies that they may have different origins. Our further statistical study indicates that brown dwarfs below this gap may primarily form in the protoplanetary disc through disc gravitational instability, while brown dwarfs above this gap may dominantly form like a stellar binary through molecular cloud fragmentation. Our discoveries have offered important insights about brown dwarf formation mechanisms and their possible relationships with planet and star formation.

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Crossref · 10.1093/mnras/stu134

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  • In Ma & Ge (2014) it is argued that two distinct brown dwarf formation mechanisms exist; BDs with masses below 42.5 Mjup are thought to be formed from a protoplanetary disc, while BDs with masses above 42.5 Mjup would form more like stellar binaries.

    “In Ma &amp; Ge (2014) it is argued that two distinct brown dwarf (BD) formation mechanisms exist; BDs with masses below 42.5 M Jup, are thought to be formed from a protoplanetary disc, while BDs with masses above 42.5 M Jup, would form more like stellar binaries.”

    From A search for transiting companions in the J1407 (V1400 Cen) system (2021) · cites this paper as Ma &amp; Ge 2014

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Research works printed but not linked: 5

  1. Ge J. et al., 2008, in Fischer D., Rasio F. A., Thorsett S. E., Wolszczan A., eds, ASP Conf. Ser. Vol. 398, Extreme Solar Systems. Astron. Soc. Pac., San Francisco, p. 449
  2. Ge J. et al., 2009, Proc. SPIE, 7440, 18
  3. Marcy G. W., Cochran W. D., Mayor M., 2000, Protostars and Planets IV. Univ. Arizona Press, Tucson, AZ
  4. Reid I. N., Metchev S. A., 2008, in Mason J. W., Dr, ed., Exoplanets. Springer-Verlag, Berlin, p. 115
  5. Sahlmann J., Ségransan D., Queloz D., Udry S., 2011a, in Sozzetti A., Lattanzi M. G., Boss A. P., eds, Proc. IAU Symp. 276, The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution. Cambridge Univ. Press, Cambridge, p. 117

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Authors
Ma, B., & Ge, J.
Affiliations
University of Florida (US)
Corresponding author
Ma, Bo
ORCID
Ma, Bo
Venue
Monthly Notices of the Royal Astronomical Society
Published
2014-02-14
Volume
439
Issue
3
Pages
2781-2789
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2087045583
Cited by
153
References
143
Citations by year
2026: 18 · 2025: 14 · 2024: 15 · 2023: 18 · 2022: 9 · 2021: 12 · 2020: 6 · 2019: 18 · 2018: 5 · 2017: 17 · 2016: 7 · 2015: 9 · 2014: 3 · 2013: 2
FWCI
6.33
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
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 › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
brown dwarfs, brown dwarf desert, molecular cloud fragmentation, eccentricity distribution, solar-type stars, exoplanets, protoplanetary disks, binary stars

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