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

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posted on 2023-07-19, 08:15 authored by AC Schneider, AJ Burgasser, J Bruursema, JA Munn, FJ Vrba, D Caselden, M Kabatnik, A Rothermich, A Sainio, TP Bickle, SE Dahm, AM Meisner, JD Kirkpatrick, G Suárez, J Gagné, JK Faherty, JM Vos, MJ Kuchner, SJ Williams, DB Gagliuffi, C Aganze, CC Hsu, C Theissen, MC Cushing, F Marocco, S Casewell
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 CH4 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 L8γ-T0γ. We tentatively find that CWISE J0506+0738 is variable at 3-5 μm 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.

History

Author affiliation

School of Physics and Astronomy, University of Leicester

Version

  • VoR (Version of Record)

Published in

Astrophysical Journal Letters

Volume

943

Issue

2

Pagination

L16

Publisher

American Astronomical Society, IOP Publishing

issn

2041-8205

eissn

2041-8213

Copyright date

2023

Available date

2023-07-19

Language

en

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