Modeling Binary Systems Containing the Hot White Dwarfs WD1136+667 and Gaia-DR2-1350
In this study, we look specifically at binary white dwarfs where the companion is a main sequence star. In particular, we look at very hot white dwarfs, many of which demonstrate the "hydrogen problem" in which modeling of their hydrogen absorption features, and optical features in general, do not appear to give accurate temperatures. The two
Wood, Hunter et al.
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2024