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Article: High-resolution radio continuum observations of compact planetary nebulae

TitleHigh-resolution radio continuum observations of compact planetary nebulae
Authors
KeywordsNebulae: Planetary
Nebulae: Structure
Stars: Radio Radiation
Issue Date1991
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X
Citation
The Astrophysical Journal, 1991, v. 378 n. 2, p. 599-610 How to Cite?
AbstractWe report 15 GHz radio continuum observations of 19 compact planetary nebulae. The high resolution (∼0″.1) images obtained allowed detailed examination of the structures of these nebulae. Most of these objects have very high radio surface brightness temperatures and critical frequencies, suggesting that they are very young planetary nebulae. Most show a "bipolar" central structure, consistent with an ellipsoidal shell viewed at an angle, and may also show extended halo structure outside of the shell, probably representing remnant material left over from the asymptotic giant branch progenitor.
Persistent Identifierhttp://hdl.handle.net/10722/179671
ISSN
2015 Impact Factor: 5.909
2015 SCImago Journal Rankings: 3.266

 

DC FieldValueLanguage
dc.contributor.authorAaquist, OBen_US
dc.contributor.authorKwok, Sen_US
dc.date.accessioned2012-12-19T10:02:44Z-
dc.date.available2012-12-19T10:02:44Z-
dc.date.issued1991en_US
dc.identifier.citationThe Astrophysical Journal, 1991, v. 378 n. 2, p. 599-610en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/179671-
dc.description.abstractWe report 15 GHz radio continuum observations of 19 compact planetary nebulae. The high resolution (∼0″.1) images obtained allowed detailed examination of the structures of these nebulae. Most of these objects have very high radio surface brightness temperatures and critical frequencies, suggesting that they are very young planetary nebulae. Most show a "bipolar" central structure, consistent with an ellipsoidal shell viewed at an angle, and may also show extended halo structure outside of the shell, probably representing remnant material left over from the asymptotic giant branch progenitor.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.subjectNebulae: Planetaryen_US
dc.subjectNebulae: Structureen_US
dc.subjectStars: Radio Radiationen_US
dc.titleHigh-resolution radio continuum observations of compact 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.doi10.1086/170461-
dc.identifier.scopuseid_2-s2.0-0042428435en_US
dc.identifier.volume378en_US
dc.identifier.issue2en_US
dc.identifier.spage599en_US
dc.identifier.epage610en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridAaquist, OB=12789145800en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US

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