A Hokupa'a/Gemini survey of the lowest mass/faintest guide stars: The very low mass binary population and its implications for brown dwarf formation theories

Laird M Close, Nick Siegler, Melanie Freed

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

Use of the highly sensitive Hokupa'a/Gemini curvature wavefront sensor has allowed, for the first time, direct adaptive optics (AO) guiding on very low mass (VLM) stars with cool spectral types (M8.0-L0.5). These low mass (Mass < 100MJupiter) objects are very cool (Teff < 3000K) and very low luminosity (V ≳ 20 at D=20 pc). However, they are red enough (V - I ∼ 4) for the Houkupa'a curvature WFS to guide on the reddest (λeff ∼ 0.8μ) photons. This is the only high angular resolution (FWHM ∼ 0.1″) survey of stars cooler than M7 from the ground. We guided on 39 such objects and detected 9 VLM binaries (7 of which were discovered for the first time to be binaries). Most of these systems (55%) are tight (separation < 5 AU) and have similar masses (ΔKs < 0.8 mag; 0.85 < q < 1.0). However, 2 systems (LHS 2397a, and 2M2331016-040618) have large ΔKs > 2.38 mag and consist of a VLM star orbited by a much cooler L6.5-L8.5 brown dwarf companion. Based on our initial flux limited (Ks < 12 mag) survey of 39 M8.0-L0.5 stars (mainly from the sample of Gizis et al. 2000) we find a binary fraction in the range 19 ± 7% for M8.0-L0.5 binaries with separations > 2.6 AU. This is slightly less than the 32 ± 9% measured for more massive (M0-M4) stars over the same separation range (Fischer & Marcy 1992). It appears M8.0-L0.5 binaries (as well as L and T dwarf binaries) have a much smaller semi-major axis distribution peak (∼ 4 AU) compared to more massive M and G stars which have a broad peak at larger ∼ 30 AU separations. We also find no VLM binaries (Mtot < 0.18M) with separations > 20 AU. We find that a velocity "kick" of ∼ 3 km/s can reproduce the observed cut-off in the semi-major axis distribution at ∼ 20 AU. This kick may have been from the VLM system being ejected from its formation mini-cluster.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
EditorsP.L. Wizinowich, D. Bonaccini
Pages1055-1064
Number of pages10
Volume4839
Edition2
DOIs
Publication statusPublished - 2002
EventAdaptive Optical System Technologies II - Waikoloa, HI, United States
Duration: Aug 22 2002Aug 26 2002

Other

OtherAdaptive Optical System Technologies II
CountryUnited States
CityWaikoloa, HI
Period8/22/028/26/02

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ASJC Scopus subject areas

  • Electrical and Electronic Engineering
  • Condensed Matter Physics

Cite this

Close, L. M., Siegler, N., & Freed, M. (2002). A Hokupa'a/Gemini survey of the lowest mass/faintest guide stars: The very low mass binary population and its implications for brown dwarf formation theories. In P. L. Wizinowich, & D. Bonaccini (Eds.), Proceedings of SPIE - The International Society for Optical Engineering (2 ed., Vol. 4839, pp. 1055-1064) https://doi.org/10.1117/12.458958