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20062025
most citedAsteroseismic inferences on GW Vir variable stars in the frame of new PG 1159 evolutionary models

117 citations · 718 across the 24 of their papers we have counts for

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Showing 2007 · astro-phShow all

5 papers · 2 filters

astro-ph2007★ 53 cited

The pulsation modes of the pre-white dwarf PG 1159-035

J. E. S. Costa, S. O. Kepler, D. E. Winget +74

PG 1159-035, a pre-white dwarf with T_eff=140,000 K, is the prototype of both two classes: the PG1159 spectroscopic class and the DOV pulsating class. Previous studies of PG 1159-0…

astro-ph2007★ 53 cited

Asteroseismological measurements on PG 1159-035, the prototype of the GW Vir variable stars

A. H. Córsico, L. G. Althaus, S. O. Kepler +2

An asteroseismological study of PG 1159-035, the prototype of the GW Vir variable stars, has been performed on the basis of detailed and full PG1159 evolutionary models presented b…

astro-ph2007★ 17 cited

On the systematics of asteroseismological mass determinations of PG1159 stars

L. G. Althaus, A. H. Córsico, S. O. Kepler +1

We analyze systematics in the asteroseismological mass determination methods in pulsating PG 1159 stars. We compare the seismic masses resulting from the comparison of the observed…

astro-ph2007★ 39 cited

Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200

A. H. Córsico, M. M. Miller Bertolami, L. G. Althaus +2

We present an asteroseismological study on PG 0122+200, the coolest known pulsating PG1159 (GW Vir) star. Our results are based on an augmented set of the full PG1159 evolutionary…

astro-ph2007★ 8 cited

Low-mass, helium-enriched PG1159 stars: a possible evolutionary origin and the implications for their pulsational stability properties

L. G. Althaus, A. H. Córsico, M. M. Miller Bertolami

We examine a recently-proposed evolutionary scenario that could explain the existence of the low-mass, helium-enriched PG1159 stars. We assess the overstability of pulsation g-mode…