Asteroseismic inferences on GW Vir variable stars in the frame of new PG 1159 evolutionary models

Abstract

This submission has been removed by arXiv administrators because it is a duplicate of astro-ph/0603735.

References in corpus (1)

• DQ white-dwarf stars with low C abundance: Possible progenitors

Cited by in corpus (8)

• Pulsating White Dwarf Stars and Precision Asteroseismology
• New nonadiabatic pulsation computations on full PG1159 evolutionary models: the theoretical GW Vir instability strip revisited
• Asteroseismological measurements on PG 1159-035, the prototype of the GW Vir variable stars
• Asteroseismological constraints on the pulsating planetary nebula nucleus (PG1159-type) RX J2117.1+3412
• Asteroseismological constraints on the coolest GW Vir variable star (PG 1159-type)PG 0122+200
• Evidence of thin helium envelopes in PG1159 stars
• On the systematics of asteroseismological mass determinations of PG1159 stars
• On the robustness of H-deficient post-AGB tracks