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Cited article:

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Monthly Notices of the Royal Astronomical Society 529 (2) 1414 (2024)
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On the Surface Helium Abundance of B-type Hot Subdwarf Stars from the WD+MS Channel of Type Ia Supernovae

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New Hot Subdwarf Stars Identified in Gaia DR2 with LAMOST DR5 Spectra. II.

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The Astrophysical Journal 881 (2) 135 (2019)
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Tidal Interactions of Close Hot Subdwarf Binaries

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Monthly Notices of the Royal Astronomical Society 481 (1) 715 (2018)
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Hydrogen in hot subdwarfs formed by double helium white dwarf mergers

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The impact of enhanced iron opacity on massive star pulsations: updated instability strips

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The blue-edge problem of the V1093 Herculis instability strip revisited using evolutionary models with atomic diffusion

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MODELS FOR METAL-POOR STARS WITH ENHANCED ABUNDANCES OF C, N, O, Ne, Na, Mg, Si, S, Ca, AND Ti, IN TURN, AT CONSTANT HELIUM AND IRON ABUNDANCES

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Slowing down atomic diffusion in subdwarf B stars: mass loss or turbulence?

Haili Hu, C. A. Tout, E. Glebbeek and M.-A. Dupret
Monthly Notices of the Royal Astronomical Society 418 (1) 195 (2011)
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