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Article: Using H 2 emission to study the fast wind in proto-planetary nebulae

TitleUsing H 2 emission to study the fast wind in proto-planetary nebulae
Authors
Hrivnak, BJSmith, NSu, KYLKelly, DMKwok, SSahai, R
KeywordsCircumstellar Matter
Planetary Nebulae: General
Stars: Agb And Post-Agb
Issue Date2006
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
Proceedings Of The International Astronomical Union, 2006, v. 2 n. 234, p. 423-424 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921306003553
AbstractWe present the results of a high-resolution H 2 imaging and spectroscopic study of four bipolar proto-planetary nebulae: IRAS 16594-4656, Hen 3-401, Rob 22, and IRAS 17150-3224. These reveal the locations and kinematics of the H 2 emission and the shaping of the nebulae by their collimated fast winds. © 2006 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/179699
ISSN
1743-9213
2020 SCImago Journal Rankings: 0.124

 

DC FieldValueLanguage
dc.contributor.authorHrivnak, BJen_US
dc.contributor.authorSmith, Nen_US
dc.contributor.authorSu, KYLen_US
dc.contributor.authorKelly, DMen_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorSahai, Ren_US
dc.date.accessioned2012-12-19T10:02:55Z-
dc.date.available2012-12-19T10:02:55Z-
dc.date.issued2006en_US
dc.identifier.citationProceedings Of The International Astronomical Union, 2006, v. 2 n. 234, p. 423-424en_US
dc.identifier.issn1743-9213en_US
dc.identifier.urihttp://hdl.handle.net/10722/179699-
dc.description.abstractWe present the results of a high-resolution H 2 imaging and spectroscopic study of four bipolar proto-planetary nebulae: IRAS 16594-4656, Hen 3-401, Rob 22, and IRAS 17150-3224. These reveal the locations and kinematics of the H 2 emission and the shaping of the nebulae by their collimated fast winds. © 2006 International Astronomical Union.en_US
dc.languageengen_US
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAUen_US
dc.relation.ispartofProceedings of the International Astronomical Unionen_US
dc.subjectCircumstellar Matteren_US
dc.subjectPlanetary Nebulae: Generalen_US
dc.subjectStars: Agb And Post-Agben_US
dc.titleUsing H 2 emission to study the fast wind in proto-planetary nebulaeen_US
dc.typeArticleen_US
dc.identifier.emailKwok, S: deannote@hku.hken_US
dc.identifier.authorityKwok, S=rp00716en_US
dc.description.naturelink_to_subscribed_fulltexten_US
dc.identifier.doi10.1017/S1743921306003553en_US
dc.identifier.scopuseid_2-s2.0-33845524248en_US
dc.identifier.volume2en_US
dc.identifier.issue234en_US
dc.identifier.spage423en_US
dc.identifier.epage424en_US
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridHrivnak, BJ=35613962100en_US
dc.identifier.scopusauthoridSmith, N=7403172437en_US
dc.identifier.scopusauthoridSu, KYL=26326482200en_US
dc.identifier.scopusauthoridKelly, DM=13104011200en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridSahai, R=7004985042en_US
dc.identifier.issnl1743-9213-

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