pith. sign in

arxiv: 1309.1500 · v2 · pith:JMLIXVNLnew · submitted 2013-09-05 · 🌌 astro-ph.SR

The Exemplar T8 Subdwarf Companion of Wolf 1130

classification 🌌 astro-ph.SR
keywords wolfj200520low-metallicitysubdwarfwisecompanionexemplarmetallicity
0
0 comments X
read the original abstract

We have discovered a wide separation (188.5") T8 subdwarf companion to the sdM1.5+WD binary Wolf 1130. Companionship of WISE J200520.38+542433.9 is verified through common proper motion over a ~3 year baseline. Wolf 1130 is located 15.83 +/- 0.96 parsecs from the Sun, placing the brown dwarf at a projected separation of ~3000 AU. Near-infrared colors and medium resolution (R~2000-4000) spectroscopy establish the uniqueness of this system as a high-gravity, low-metallicity benchmark. Although there are a number of low-metallicity T dwarfs in the literature, WISE J200520.38+542433.9 has the most extreme inferred metallicity to date with [Fe/H] = -0.64 +/- 0.17 based on Wolf 1130. Model comparisons to this exemplar late-type subdwarf support it having an old age, a low metallicity, and a small radius. However, the spectroscopic peculiarities of WISE J200520.38+542433.9 underscore the importance of developing the low-metallicity parameter space of the most current atmospheric models.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction

    astro-ph.IM 2026-05 unverdicted novelty 6.0

    ROSSINI achieves integral field spectroscopy without IFUs through rotational slitless spectroscopy combined with tomographic reconstruction, recovering input datacubes to percent accuracy in numerical simulations.