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Conference Paper: Evolution from the asymptotic giant branch to planetary nebulae

TitleEvolution from the asymptotic giant branch to planetary nebulae
Authors
KeywordsAgb And Post-Agb Stars
Planetary Nebulae
Stellar Winds
Issue Date2005
Citation
Aip Conference Proceedings, 2005, v. 804, p. 187-196 How to Cite?
AbstractThe post-asymptotic-giant-branch (post-AGB) or pre-planetary nebulae (PPN) phase of stellar evolution plays an important role in the dynamical shaping of PNe. While the interacting stellar winds model has achieved tremendous success in the explaining of the 1-D structures (shells, crowns, haloes) of PNe, the origins of arcs, rings, and multipolar structures remain a mystery. The synthesis of gas-phase molecules and solid-state compounds that begin in the stellar winds from AGB stars also undergo significant evolution during the post-AGB phase. Organic compounds of both aliphatic and aromatic structures are produced, which carries significant implications on the chemical enrichment of the interstellar medium. © 2005 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/179622
ISSN
References

 

DC FieldValueLanguage
dc.contributor.authorKwok, Sen_US
dc.date.accessioned2012-12-19T10:01:39Z-
dc.date.available2012-12-19T10:01:39Z-
dc.date.issued2005en_US
dc.identifier.citationAip Conference Proceedings, 2005, v. 804, p. 187-196en_US
dc.identifier.issn0094-243Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/179622-
dc.description.abstractThe post-asymptotic-giant-branch (post-AGB) or pre-planetary nebulae (PPN) phase of stellar evolution plays an important role in the dynamical shaping of PNe. While the interacting stellar winds model has achieved tremendous success in the explaining of the 1-D structures (shells, crowns, haloes) of PNe, the origins of arcs, rings, and multipolar structures remain a mystery. The synthesis of gas-phase molecules and solid-state compounds that begin in the stellar winds from AGB stars also undergo significant evolution during the post-AGB phase. Organic compounds of both aliphatic and aromatic structures are produced, which carries significant implications on the chemical enrichment of the interstellar medium. © 2005 American Institute of Physics.en_US
dc.languageengen_US
dc.relation.ispartofAIP Conference Proceedingsen_US
dc.subjectAgb And Post-Agb Starsen_US
dc.subjectPlanetary Nebulaeen_US
dc.subjectStellar Windsen_US
dc.titleEvolution from the asymptotic giant branch to planetary nebulaeen_US
dc.typeConference_Paperen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1063/1.2146271en_US
dc.identifier.scopuseid_2-s2.0-33751227822en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-33751227822&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume804en_US
dc.identifier.spage187en_US
dc.identifier.epage196en_US
dc.publisher.placeUnited Statesen_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US

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