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- Publisher Website: 10.1063/1.2146271
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Conference Paper: Evolution from the asymptotic giant branch to planetary nebulae
Title | Evolution from the asymptotic giant branch to planetary nebulae |
---|---|
Authors | |
Keywords | Agb And Post-Agb Stars Planetary Nebulae Stellar Winds |
Issue Date | 2005 |
Publisher | American Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/ |
Citation | AIP Conference Proceedings, 2005, v. 804 n. 1, p. 187-196 How to Cite? |
Abstract | The 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 Identifier | http://hdl.handle.net/10722/179622 |
ISSN | 2023 SCImago Journal Rankings: 0.152 |
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kwok, S | en_US |
dc.date.accessioned | 2012-12-19T10:01:39Z | - |
dc.date.available | 2012-12-19T10:01:39Z | - |
dc.date.issued | 2005 | en_US |
dc.identifier.citation | AIP Conference Proceedings, 2005, v. 804 n. 1, p. 187-196 | - |
dc.identifier.issn | 0094-243X | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/179622 | - |
dc.description.abstract | The 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.language | eng | en_US |
dc.publisher | American Institute of Physics. The Journal's web site is located at http://proceedings.aip.org/ | - |
dc.relation.ispartof | AIP Conference Proceedings | en_US |
dc.subject | Agb And Post-Agb Stars | en_US |
dc.subject | Planetary Nebulae | en_US |
dc.subject | Stellar Winds | en_US |
dc.title | Evolution from the asymptotic giant branch to planetary nebulae | en_US |
dc.type | Conference_Paper | en_US |
dc.identifier.email | Kwok, S: deannote@hku.hk | en_US |
dc.identifier.authority | Kwok, S=rp00716 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1063/1.2146271 | en_US |
dc.identifier.scopus | eid_2-s2.0-33751227822 | en_US |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-33751227822&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 804 | en_US |
dc.identifier.issue | 1 | - |
dc.identifier.spage | 187 | en_US |
dc.identifier.epage | 196 | en_US |
dc.publisher.place | United States | en_US |
dc.identifier.scopusauthorid | Kwok, S=22980498300 | en_US |
dc.identifier.issnl | 0094-243X | - |