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Asymmetric Nightside CO2 Features, Inefficient Heat Transport, and Precise Evolutionary Constraints: Spectroscopic Phase Curves Reveal the Past and Present of a White Dwarf–Brown Dwarf Binary

  • Authors: Daphne Broski-Laing, Yifan Zhou, Joshua D. Lothringer, Daniel Apai, Jenni R. French, Sarah L. Casewell, L. C. Mayorga, Lael Shin, Ben W. P. Lew, Xianyu Tan, Vivien Parmentier, Siyi Xu, Mark S. Marley

Daphne Broski-Laing et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 8.

Illustration of the WD–BD geometry at eight representative phases in the orbit. The upper illustrations visualize a simple representation of the brown dwarf hemisphere observed at each phase. The shading indicates how much of the dayside (pink) and nightside (purple) hemispheres are visible at each phase. In phases (A) and (E) (nightside and dayside), the smaller central circle indicates when the white dwarf is behind or in front of the brown dwarf. The center panel shows the phase-folded, broadband phase curve. The highlights indicate the amount of time used to produce each median-combined spectrum for each of the eight representative phases. Each of the eight highlighted phases is also shown in the lower orbital diagram, where the inclination is adjusted to show all phases of the orbit more clearly.

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