WD 1856+534 is part of a multiple system including a pair of M dwarf stars (G 229-20 AB) 1081 AUs away. The low-mass pair is in turn separated by about 56 AUs.
Modelling the 3D atmospheric structure of the cold Jupiter WD1856+534b orbiting a white dwarf
NOTI P., LEE E., KITZMANN D., MacDONALD R., JENKINS S. et al.
MNRAS
, in press
paperarxiv
Transit Timing of the White Dwarf-Cold Jupiter System WD 1856+534
GENDREAU-DISTLER A., BOSTOW K., PATRA K., ALVARADO III E., BETZ A. et al.
ApJ. Letters
, submitted
arxiv
Probing the Dynamical History of a White Dwarf Planet
JENKINS S., BLOUIN S., GAO P., LIMBACH M., MacDONALD R. et al.
JWST Proposal. Cycle 4
, ID. #9157
JWST GO Proposal 9157
By the Ashes of Stars: A Chemical Census of a White Dwarf Planet
MacDONALD R., BATALHA N., BLOUIN S., BOEHM V., FOOTE T. et al.
JWST Proposal. Cycle 4
, ID. #9033
JWST GO 9033
A high stellar multiplicity rate amongst TESS planet candidates in the Neptunian desert using Gaia DR3 astrometry
EELES-NOLLE F. & ARMSTRONG D.
MNRAS
, 541
, 1419
paperarxiv
The ouput simulation data of the Exo-FMS GCM and of the post-processing with gCMCRT for Modelling the 3D atmospheric structure of the cold Jupiter WD1856+534b orbiting a white dwarf