Metal abundances in hot white dwarfs with signatures of a superionized wind

K. Werner; T. Rauch; J. W. Kruk

doi:10.1051/0004-6361/201731740

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Volume 609 (January 2018)

A&A, 609 (2018) A107

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Fig. 9

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FUSE spectrum of the DO HS 0727+6003, similar to Fig. 1. Model: T_eff = 65 000 K, log g = 7.5 (same one as for HS 0713+3958 in Fig. 5).

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