On the excitation of PG1159-type pulsations

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Accepted for publication in Astronomy & Astrophysics

Scientific paper

10.1051/0004-6361:20042486

Stability properties are presented of dipole and quadrupole nonradial
oscillation modes of model stars that experienced a late helium shell flash on
their way to the white-dwarf cooling domain. The computed instability domains
are compared with the observed hot variable central stars of planetary nebulae
and the GW Vir pulsators.

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