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Article: Infrared Space Observatory observations of the unidentified 30 micron feature in proto-planetary nebulae

TitleInfrared Space Observatory observations of the unidentified 30 micron feature in proto-planetary nebulae
Authors
KeywordsCircumstellar Matter
Infrared: Stars
Ism: Lines And Bands
Planetary Nebulae: General
Radiative Transfer
Stars: Agb And Post-Agb
Issue Date2002
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X
Citation
The Astrophysical Journal, 2002, v. 567 n. 1 pt. 1, p. 412-422 How to Cite?
AbstractThe intrinsic emission profile of the unidentified broad 30 μm emission feature is derived from Infrared Space Observatory (ISO) spectra of proto-planetary nebulae (PPNs). The feature is resolved into two components: a narrower feature at 26 μm and a broader feature at 33 μm. The intrinsic profiles of these two features and their varying strengths in PPNs are determined. The chemical origin of these features and the processes responsible for their changing strengths from asymptotic giant branch (AGB) stars to PPNs to planetary nebulae are discussed.
Persistent Identifierhttp://hdl.handle.net/10722/179643
ISSN
2015 Impact Factor: 5.909
2015 SCImago Journal Rankings: 3.266
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorVolk, Ken_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorHrivnak, BJen_US
dc.contributor.authorSzczerba, Ren_US
dc.date.accessioned2012-12-19T10:02:13Z-
dc.date.available2012-12-19T10:02:13Z-
dc.date.issued2002en_US
dc.identifier.citationThe Astrophysical Journal, 2002, v. 567 n. 1 pt. 1, p. 412-422en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/179643-
dc.description.abstractThe intrinsic emission profile of the unidentified broad 30 μm emission feature is derived from Infrared Space Observatory (ISO) spectra of proto-planetary nebulae (PPNs). The feature is resolved into two components: a narrower feature at 26 μm and a broader feature at 33 μm. The intrinsic profiles of these two features and their varying strengths in PPNs are determined. The chemical origin of these features and the processes responsible for their changing strengths from asymptotic giant branch (AGB) stars to PPNs to planetary nebulae are discussed.en_US
dc.languageengen_US
dc.publisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637Xen_US
dc.relation.ispartofThe Astrophysical Journalen_US
dc.rightsCreative Commons: Attribution 3.0 Hong Kong License-
dc.subjectCircumstellar Matteren_US
dc.subjectInfrared: Starsen_US
dc.subjectIsm: Lines And Bandsen_US
dc.subjectPlanetary Nebulae: Generalen_US
dc.subjectRadiative Transferen_US
dc.subjectStars: Agb And Post-Agben_US
dc.titleInfrared Space Observatory observations of the unidentified 30 micron feature in proto-planetary nebulaeen_US
dc.typeArticleen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturepublished_or_final_versionen_US
dc.identifier.doi10.1086/337992en_US
dc.identifier.scopuseid_2-s2.0-0009868005en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-0009868005&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume567en_US
dc.identifier.issue1 pt. 1en_US
dc.identifier.spage412en_US
dc.identifier.epage422en_US
dc.identifier.isiWOS:000174047700038-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridVolk, K=7006571965en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridHrivnak, BJ=35613962100en_US
dc.identifier.scopusauthoridSzczerba, R=7004424914en_US

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