The Astrophysical Journal Letters (Jan 2023)

Redder than Red: Discovery of an Exceptionally Red L/T Transition Dwarf

  • Adam C. Schneider,
  • Adam J. Burgasser,
  • Justice Bruursema,
  • Jeffrey A. Munn,
  • Frederick J. Vrba,
  • Dan Caselden,
  • Martin Kabatnik,
  • Austin Rothermich,
  • Arttu Sainio,
  • Thomas P. Bickle,
  • Scott E. Dahm,
  • Aaron M. Meisner,
  • J. Davy Kirkpatrick,
  • Genaro Suárez,
  • Jonathan Gagné,
  • Jacqueline K. Faherty,
  • Johanna M. Vos,
  • Marc J. Kuchner,
  • Stephen J. Williams,
  • Daniella Bardalez Gagliuffi,
  • Christian Aganze,
  • Chih-Chun Hsu,
  • Christopher Theissen,
  • Michael C. Cushing,
  • Federico Marocco,
  • Sarah Casewell,
  • The Backyard Worlds: Planet 9 Collaboration

DOI
https://doi.org/10.3847/2041-8213/acb0cd
Journal volume & issue
Vol. 943, no. 2
p. L16

Abstract

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We present the discovery of CWISE J050626.96+073842.4 (CWISE J0506+0738), an L/T transition dwarf with extremely red near-infrared colors discovered through the Backyard Worlds: Planet 9 citizen science project. Photometry from UKIRT and CatWISE give a ( J − K ) _MKO color of 2.97 ± 0.03 mag and a J _MKO − W2 color of 4.93 ± 0.02 mag, making CWISE J0506+0738 the reddest known free-floating L/T dwarf in both colors. We confirm the extremely red nature of CWISE J0506+0738 using Keck/NIRES near-infrared spectroscopy and establish that it is a low-gravity, late-type L/T transition dwarf. The spectrum of CWISE J0506+0738 shows possible signatures of CH _4 absorption in its atmosphere, suggesting a colder effective temperature than other known, young, red L dwarfs. We assign a preliminary spectral type for this source of L8 γ –T0 γ . We tentatively find that CWISE J0506+0738 is variable at 3–5 μ m based on multiepoch WISE photometry. Proper motions derived from follow-up UKIRT observations combined with a radial velocity from our Keck/NIRES spectrum and a photometric distance estimate indicate a strong membership probability in the β Pic moving group. A future parallax measurement will help to establish a more definitive moving group membership for this unusual object.

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