Abstract
We report the discovery of two faint ultracool companions to the nearby (d ∼ 17.9 pc) young G2 V star HD 130948 (HR 5534, HIP 72567) using the Hokupa'a adaptive optics (AO) instrument mounted on the Gemini North 8 m telescope. Both objects have the same common proper motion as the primary star as seen over a 7 month baseline and have near-IR photometric colors that are consistent with an early L classification. Near-IR spectra taken with the NIRSPEC AO instrument on the Keck II telescope reveal K I lines, FeH, and H 2O band heads. Based on these spectra, we determine that both objects have a spectral type of dL2 with an uncertainty of two spectral subclasses. The position of the new companions on the H-R diagram in comparison with theoretical models is consistent with the young age of the primary star (<0.8 Gyr) estimated on the basis of X-ray activity, lithium abundance, and fast rotation. HD 130948B and C likely constitute a pair of young contracting brown dwarfs with an orbital period of about 10 yr and will yield dynamical masses for L dwarfs in the near future.
| Original language | English (US) |
|---|---|
| Pages (from-to) | L133-L136 |
| Journal | Astrophysical Journal |
| Volume | 567 |
| Issue number | 2 II |
| DOIs | |
| State | Published - Mar 10 2002 |
| Externally published | Yes |
Keywords
- Binaries: close
- Binaries: visual
- Stars: evolution
- Stars: fundamental parameters
- Stars: imaging
- Stars: low-mass, brown dwarfs
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
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