
© Burgasser et al., 2024.Forward modeling of the Keck/NIRES spectrum of J1249+3621 in the 1.10–1.19 µm (left), and 1.235–1.28 µm (right) spectral regions, both of which contain stellar and telluric absorption features.
Using the Keck II telescope, astronomers have detected an object that may be a brown dwarf or a low-mass star, exhibiting a very high radial velocity. The object, designated CWISE J124909.08+362116.0 is located some 400 light years away. The finding was
reported July 11 on the pre-print server arXiv.
Brown dwarfs (BDs) are intermediate objects between planets and stars, occupying the mass range between 13 and 80 Jupiter masses (0.012 and 0.076 solar masses). They form like stars but are not sufficiently massive to sustain hydrogen fusion in their cores.
Now, a team of astronomers led by Adam Burgasser of the University of California San Diego reports
the detection of a new object at the brown dwarf/star mass boundary.Using the Near-Infrared Echellette Spectrometer (NIRES) at the Keck II telescope, they investigated CWISE J124909.08+362116.0 (or CWISE J1249+3621 for short) — a high proper motion faint red source first identified by citizen scientists. As a result, it turned out that the source is a rare type of hypervelocity subdwarf.
"We report the discovery of a high velocity, very low-mass star or brown dwarf whose kinematics suggest it is unbound to the Milky Way. (...) The fastest 'hypervelocity' stars are unbound to the Milky Way's gravitational potential and may even have extragalactic origins," the researchers explained.
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