The far-ultraviolet spectra of two hot PG 1159 stars

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Table 3

Asteroseismic, spectroscopic, and initial masses of the five considered PG 1159 stars.

Star	M_puls/M_⊙	M_spec/M_⊙	M_init/M_⊙ ^(e)

PG 1424+535	–	^(c)	≈1–2
PG 1707+427	^(a)	^(c)	≈1–3
PG 1159−035	^(b)	^(c)	≈1–2
PG 1144+005	–	^(d)	≈1–2.5
PG 1520+525	–	^(d)	≈1–4

Reference.

^(a)

Córsico et al. (2008);

^(b)

Córsico et al. (2009);

^(c)

Werner & Rauch (2014);

^(d)

this work;

^(e)

estimated from initial-to-final mass relation of Weidemann (2000) using M_spec.

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