Improved infrared photometry and a preliminary parallax measurement for the extremely cold brown dwarf CWISEP J144606.62231717.8
arXiv:1912.07692 · doi:10.3847/2041-8213/ab6201
Abstract
We present follow-up observations at 3.6m (ch1) and 4.5m (ch2) of CWISEP J144606.62231717.8, one of the coldest known brown dwarfs in the solar neighborhood. This object was found by mining the Wide-field Infrared Survey Explorer () and data via the CatWISE Preliminary Catalog by Meisner et al. (2019b), where an initial color of ch1ch2 = 3.710.44 mag was reported, implying it could be one of the reddest, and hence coldest, known brown dwarfs. Additional data presented here allows us to revise its color to ch1ch2 = 2.9860.048 mag, which makes CWISEP J144606.62231717.8 the 5th reddest brown dwarf ever observed. A preliminary trigonometric parallax measurement, based on a combination of and astrometry, places this object at a distance of 10.1 pc. Based on our improved color and preliminary parallax, CWISEP J144606.62231717.8 has a in the 310360 K range. Assuming an age of 0.513 Gyr, this corresponds to a mass between 2 and 20 .
Accepted by ApJL. 8 pages, 3 figures, 1 table
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Cited by in corpus (8)
- The CatWISE2020 Catalog
- The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs
- Spitzer Follow-up of Extremely Cold Brown Dwarfs Discovered by the Backyard Worlds: Planet 9 Citizen Science Project
- unTimely: a Full-sky, Time-Domain unWISE Catalog
- Self-consistent Models of Y Dwarf Atmospheres with Water Clouds and Disequilibrium Chemistry
- Expanding the Y Dwarf Census with Spitzer Follow-up of the Coldest CatWISE Solar Neighborhood Discoveries
- WISEA J083011.95+283716.0: A Missing Link Planetary-Mass Object
- An Improved Near-Infrared Spectrum of the Archetype Y Dwarf WISEP J182831.08+265037.8