WISEA J064750.85-154616.4: a new nearby L/T transition dwarf
arXiv:1406.1005 · doi:10.1051/0004-6361/201424070
Abstract
Aims: Our aim is to detect and classify previously overlooked brown dwarfs in the solar neighbourhood. Methods: We performed a proper motion search among bright sources observed with the Wide-field Infrared Survey Explorer (WISE) that are also seen in the Two Micron All Sky Survey (2MASS). Our candidates appear according to their red colours as nearby late-L dwarf candidates. Low-resolution near-infrared (NIR) classification spectroscopy in the band allowed us to get spectroscopic distance and tangential velocity estimates. Results: We have discovered a new L9.5 dwarf, WISEA J064750.85-154616.4, at a spectroscopic distance of about 14 pc and with a tangential velocity of about 11 km/s, typical of the Galactic thin disc population. We have confirmed another recently found L/T transition object at about 10 pc, WISEA J140533.13+835030.7, which we classified as L8 (NIR).
Research Note accepted for publication in Astronomy and Astrophysics, 5 pages, 3 figures
References in corpus (5)
- Discovery of a ~250 K Brown Dwarf at 2 pc from the Sun
- Discovery of 11 New T Dwarfs in the Two Micron All-Sky Survey, Including a Possible L/T Transition Binary
- Doppler Imaging of Exoplanets and Brown Dwarfs
- The Brown dwarf Atmosphere Monitoring (BAM) Project I: The largest near-IR monitoring survey of L- & T-dwarfs
- Characterization of High Proper Motion Objects from the Wide-field Infrared Survey Explorer
Cited by in corpus (6)
- The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs
- The 10 parsec sample in the Gaia era
- A Volume-Limited Sample of Ultracool Dwarfs. I. Construction, Space Density, and a Gap in the L/T Transition
- The Hawaii Infrared Parallax Program. IV. A Comprehensive Parallax Survey of L0-T8 dwarfs with UKIRT
- A Brown Dwarf Census from the SIMP Survey
- Properties of the solar neighbor WISE J072003.20-084651.2