ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion

Details ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion

2002-09-20

arxiv.org/abs/astro-ph/0209427v1

Astronomy and Astrophysics

Astrophysics

1 page, 1 EPS figure, to appear in RevMxAA (SC), poster proceeding

Scientific paper

The "born-again" PNe V605 Aql (A58) and V4344 Sgr (Sakurai) give us the rare chance to follow shell formation and building of the winds in "real-time". The high carbon abundance, and thus the high dust formation rate, enhances the mechanisms. Thus the timescales are shortened. My data presented here gives a quick look on the results of new observations of V605 Aql and its old planetary nebula (PN) A58 obtained at the ESO NTT (August 2002).

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