The importance of the remnant's mass for VLTP born again times. Implications for V4334 Sgr and V605 Aql.

MILLER BERTOLAMI M. M. AND ALTHAUS L. G.

Tuebingen, Alemania

Conferencia; Hydrogen-Deficient Stars; 2007

Institute for Astronomy and Astrophysics at the University of Tübingen

Abstract. We present numerical simulations of the very late thermal pulse (VLTP) scenario for a wide range of remnant masses. We show that, by taking into account the di erent possible remnant masses, the fast outburst evolution of V4334 Sgr (a.k.a. Sakurai's Object) and V605 Aql can be reproduced within standard 1D stellar evolution models. A dichotomy in the born again timescales is found, with lower mass remnants evolving in a few years and higher mass remnants (M 0.6 M ) failing to expand due to the H- ash and, as a consequence, evolving in timescales typical of He-shell  ash driven born agains (  100 yr).