J2102-4145 shows one 0.375-solar-mass white dwarf retaining a thick hydrogen envelope via stable mass transfer and a 0.314-solar-mass companion with an extremely thin envelope below 10^{-7} solar masses after common-envelope ejection, challenging standard bifurcation criteria.
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2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
ZTF-discovered radial-mode sdB pulsators have mean Teff of 28,300 K and log g of 5.56, placing them at the boundary between V361 Hya and V1093 Her classes with canonical masses and distinguishing them from blue large-amplitude pulsators.
citing papers explorer
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Extreme mass loss during common envelope evolution: the origin of the double low-mass white dwarf system J2102--4145
J2102-4145 shows one 0.375-solar-mass white dwarf retaining a thick hydrogen envelope via stable mass transfer and a 0.314-solar-mass companion with an extremely thin envelope below 10^{-7} solar masses after common-envelope ejection, challenging standard bifurcation criteria.
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Spectroscopic follow-up of hot subdwarf variables found in ZTF -- Atmospheric and fundamental properties of radial-mode sdB pulsators
ZTF-discovered radial-mode sdB pulsators have mean Teff of 28,300 K and log g of 5.56, placing them at the boundary between V361 Hya and V1093 Her classes with canonical masses and distinguishing them from blue large-amplitude pulsators.