Bibcode
Lodieu, N.; Zapatero Osorio, M. R.; Rebolo, R.; Béjar, V. J. S.; Pavlenko, Y.; Pérez-Garrido, A.
Bibliographical reference
Astronomy and Astrophysics, Volume 581, id.A73, 11 pp.
Advertised on:
9
2015
Journal
Citations
22
Refereed citations
21
Description
Aims: The aim of the project is to characterise the two
components of the brown dwarf system nearest to the Sun, WISE
J104915.57-531906.1 (also called Luhman 16AB) at optical and
near-infrared wavelengths. Methods: We obtained high
signal-to-noise intermediate-resolution (R ~ 6000-11 000) optical
(600-1000 nm) and near-infrared (1000-2480 nm) spectra of each component
of Luhman 16AB with the X-Shooter instrument on the Very Large
Telescope. Results: We classify the primary and secondary of the
Luhman 16 system as L6-L7.5 and T0±1, respectively, in agreement
with previous measurements published in the literature. We present
measurements of the lithium pseudo-equivalent widths, which appear of
similar strength in both components (8.2 ± 1.0 Å for the L
and 8.4 ± 1.5 Å for the T component). The presence of
lithium (7Li) in both components implies masses lower than
0.06 M⊙, while the comparison with models suggests lower
limits of 0.04 M⊙. The detection of lithium in the T
component is the first of its kind. Similarly, we assess the strength of
other alkali lines (e.g. pseudo-equivalent widths of 6-7 Å for RbI
and 4-7 Å for CsI) present in the optical and near-infrared
regions and compare with estimates for L and T dwarfs. We also derive
effective temperatures and luminosities of each component of the binary:
-4.66 ± 0.08 dex and 1305 K for the L dwarf and -4.68 ±
0.13 dex and 1320 K for the T dwarf. According to our radial velocity
determinations, the binary does not appear to belong to any of the
well-known moving group. Our preliminary theoretical analysis of the
optical and J-band spectra indicates that the L- and T-type spectra can
be reproduced with a single temperature and gravity but different
relative chemical abundances, which strongly affects the spectral energy
distribution of L/T transition objects.
Based on observations collected at the European Southern Observatory,
Chile, under DDT programme 290.C-5200(B) (PI Lodieu).FITS files of the
reduced spectra are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr
(ftp://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/581/A73
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