Does GD 356 have a Terrestrial Planetary Companion?
Dayal T. Wickramasinghe, Jay Farihi, Christopher A. Tout, Lilia, Ferrario, Richard J. Stancliffe

TL;DR
This paper investigates whether GD 356, a magnetic white dwarf with unique emission lines, has a planetary companion, using infrared observations and revisiting models of its heating mechanism.
Contribution
It provides new upper limits on potential planetary companions and critically evaluates existing models, proposing a white dwarf merger origin for the system.
Findings
No companion above 12 Jupiter masses detected
Excludes accretion-based models for the heating mechanism
Suggests a planetary system formed from a white dwarf merger
Abstract
GD 356 is unique among magnetic white dwarfs because it shows Zeeman-split Balmer lines in pure emission. The lines originate from a region of nearly uniform field strength (delta B/B is approximately 0.1) that covers 10 per cent of the stellar surface in which there is a temperature inversion. The energy source that heats the photosphere remains a mystery but it is likely to be associated with the presence of a companion. Based on current models we use archival Spitzer IRAC observations to place a new and stringent upper limit of 12 Jupiter masses for the mass of such a companion. In the light of this result and the recent discovery of a 115 min photometric period for GD 356, we exclude previous models that invoke accretion and revisit the unipolar inductor model that has been proposed for this system. In this model a highly conducting planet with a metallic core orbits the magnetic…
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