Common envelope evolution and triple dynamics as potential pathways to form the inner white dwarf + brown dwarf binary of the triple star system Gaia 0007−1605
Date Issued
2023-02
Author(s) USM
DOI
10.1093/mnras/stac3675
Abstract
The recently discovered system Gaia 0007-1605 consisting of a white dwarf (WD) with a close brown dwarf companion and a distant WD tertiary very much resembles the triple system containing the first transiting planet candidate around a WD ever discovered:
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