V605 Aq1 and A58

Details V605 Aq1 and A58 V605 Aq1 and A58

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ans...324..140l&link_type=abstract

Astronomische Nachrichten, Supplementary Issue 3, Vol. 324, Short Contributions of the Annual Scientific Meeting of the Astronom

Astronomy and Astrophysics

Astronomy

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. The high carbon abundance, and thus the high dust formation rate, enhances the mechanisms (Koller & Kimeswenger 2001). Thus the timescales are shortened. Our data presented here gives a quick look on the results of the observations of V605 Aql and its old planetary nebula (PN) A58 obtained at the ESO NTT (August 2002). We also intend to include preliminary results of new data, which we will obtain in July 2003.

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