ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion
| dc.creator | Kimeswenger, S. | |
| dc.date | 2002-09-20 | |
| dc.date.accessioned | 2026-07-07T02:05:20Z | |
| dc.date.available | 2026-07-07T02:05:20Z | |
| dc.description | 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). | |
| dc.description | 1 page, 1 EPS figure, to appear in RevMxAA (SC), poster proceeding | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0209427 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0209427 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/5071 | |
| dc.subject | Astrophysics | |
| dc.title | ate helium flash in V605 Aql: PNe evolution and shell formation in quick motion | |
| dc.type | text |