Discovery of the Remarkably Red L/T Transition Object VHS J183135.58-551355.9

Fuente: arXiv
Saved in:
Bibliographic Details
Main Authors: Bickle, Thomas P., Schneider, Adam C., Gagné, Jonathan, Faherty, Jacqueline K., Rothermich, Austin, Vos, Johanna M., Suárez, Genaro, Kirkpatrick, J. Davy, Meisner, Aaron M., Kuchner, Marc J., Burgasser, Adam J., Marocco, Federico, Casewell, Sarah L., Caselden, Dan, Gagliuffi, Daniella Bardalez, Worlds, The Backyard, :, Collaboration, Planet 9
Format: Preprint
Published: 2024
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866909192444444672
author Bickle, Thomas P.
Schneider, Adam C.
Gagné, Jonathan
Faherty, Jacqueline K.
Rothermich, Austin
Vos, Johanna M.
Suárez, Genaro
Kirkpatrick, J. Davy
Meisner, Aaron M.
Kuchner, Marc J.
Burgasser, Adam J.
Marocco, Federico
Casewell, Sarah L.
Caselden, Dan
Gagliuffi, Daniella Bardalez
Worlds, The Backyard
:
Collaboration, Planet 9
author_facet Bickle, Thomas P.
Schneider, Adam C.
Gagné, Jonathan
Faherty, Jacqueline K.
Rothermich, Austin
Vos, Johanna M.
Suárez, Genaro
Kirkpatrick, J. Davy
Meisner, Aaron M.
Kuchner, Marc J.
Burgasser, Adam J.
Marocco, Federico
Casewell, Sarah L.
Caselden, Dan
Gagliuffi, Daniella Bardalez
Worlds, The Backyard
:
Collaboration, Planet 9
contents We present the discovery of VHS J183135.58$-$551355.9 (hereafter VHS J1831$-$5513), an L/T transition dwarf identified as a result of its unusually red near-infrared colors ($J-K_{\rm S}=3.633\pm0.277$ mag; $J-W2=6.249\pm0.245$ mag) from the VISTA Hemisphere Survey and CatWISE2020 surveys. We obtain low resolution near-infrared spectroscopy of VHS J1831$-$5513 using Magellan/FIRE to confirm its extremely red nature and assess features sensitive to surface gravity (i.e., youth). Its near-infrared spectrum shows multiple CH$_{\rm 4}$ absorption features, indicating an exceptionally low effective temperature for its spectral type. Based on proper motion measurements from CatWISE2020 and a photometric distance derived from its $K_{\rm S}$-band magnitude, we find that VHS J1831$-$5513 is a likely ($\sim$85$\%$ probability) kinematic member of the $β$ Pictoris moving group. Future radial velocity and trigonometric parallax measurements will clarify such membership. Follow-up mid-infrared or higher resolution near-infrared spectroscopy of this object will allow for further investigation as to the cause(s) of its redness, such as youth, clouds, and viewing geometry.
format Preprint
id arxiv_https___arxiv_org_abs_2405_03849
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Discovery of the Remarkably Red L/T Transition Object VHS J183135.58-551355.9
Bickle, Thomas P.
Schneider, Adam C.
Gagné, Jonathan
Faherty, Jacqueline K.
Rothermich, Austin
Vos, Johanna M.
Suárez, Genaro
Kirkpatrick, J. Davy
Meisner, Aaron M.
Kuchner, Marc J.
Burgasser, Adam J.
Marocco, Federico
Casewell, Sarah L.
Caselden, Dan
Gagliuffi, Daniella Bardalez
Worlds, The Backyard
:
Collaboration, Planet 9
Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
We present the discovery of VHS J183135.58$-$551355.9 (hereafter VHS J1831$-$5513), an L/T transition dwarf identified as a result of its unusually red near-infrared colors ($J-K_{\rm S}=3.633\pm0.277$ mag; $J-W2=6.249\pm0.245$ mag) from the VISTA Hemisphere Survey and CatWISE2020 surveys. We obtain low resolution near-infrared spectroscopy of VHS J1831$-$5513 using Magellan/FIRE to confirm its extremely red nature and assess features sensitive to surface gravity (i.e., youth). Its near-infrared spectrum shows multiple CH$_{\rm 4}$ absorption features, indicating an exceptionally low effective temperature for its spectral type. Based on proper motion measurements from CatWISE2020 and a photometric distance derived from its $K_{\rm S}$-band magnitude, we find that VHS J1831$-$5513 is a likely ($\sim$85$\%$ probability) kinematic member of the $β$ Pictoris moving group. Future radial velocity and trigonometric parallax measurements will clarify such membership. Follow-up mid-infrared or higher resolution near-infrared spectroscopy of this object will allow for further investigation as to the cause(s) of its redness, such as youth, clouds, and viewing geometry.
title Discovery of the Remarkably Red L/T Transition Object VHS J183135.58-551355.9
topic Solar and Stellar Astrophysics
Earth and Planetary Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2405.03849