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Article: Hubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disk

TitleHubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disk
Authors
KeywordsCircumstellar Matter
Planetary Nebulae: General
Stars: Agb And Post-Agb
Issue Date1998
PublisherInstitute of Physics Publishing Ltd. The Journal's web site is located at http://iopscience.iop.org/0004-637X
Citation
The Astrophysical Journal, 1998, v. 508 n. 2 pt. 2, p. 744-751 How to Cite?
AbstractThe bipolar proto-planetary nebula IRAS 17441-2411 (the "Silkworm Nebula") was observed with the Hubble Space Telescope. By fitting the observed spectral energy distribution and the V-band image by a two-dimensional radiation transfer model, we derive the properties of the circumstellar wind and a proposed circumstellar "disk." We suggest that bipolar structures are probably more common than actually observed, because objects with similar intrinsic structures may simply appear stellar because of their orientation in the sky. © 1998. The American Astronomical Society. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/179687
ISSN
2015 Impact Factor: 5.909
2015 SCImago Journal Rankings: 3.266
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorSu, KYLen_US
dc.contributor.authorVolk, Ken_US
dc.contributor.authorKwok, Sen_US
dc.contributor.authorHrivnak, BJen_US
dc.date.accessioned2012-12-19T10:02:50Z-
dc.date.available2012-12-19T10:02:50Z-
dc.date.issued1998en_US
dc.identifier.citationThe Astrophysical Journal, 1998, v. 508 n. 2 pt. 2, p. 744-751en_US
dc.identifier.issn0004-637Xen_US
dc.identifier.urihttp://hdl.handle.net/10722/179687-
dc.description.abstractThe bipolar proto-planetary nebula IRAS 17441-2411 (the "Silkworm Nebula") was observed with the Hubble Space Telescope. By fitting the observed spectral energy distribution and the V-band image by a two-dimensional radiation transfer model, we derive the properties of the circumstellar wind and a proposed circumstellar "disk." We suggest that bipolar structures are probably more common than actually observed, because objects with similar intrinsic structures may simply appear stellar because of their orientation in the sky. © 1998. The American Astronomical Society. All rights reserved.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.subjectPlanetary Nebulae: Generalen_US
dc.subjectStars: Agb And Post-Agben_US
dc.titleHubble space telescope imaging of iras 17441-2411: A case study of a bipolar nebula with a circumstellar disken_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.doi10.1086/306449en_US
dc.identifier.scopuseid_2-s2.0-22444453855en_US
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-22444453855&selection=ref&src=s&origin=recordpageen_US
dc.identifier.volume508en_US
dc.identifier.issue2 pt. 2en_US
dc.identifier.spage744en_US
dc.identifier.epage751en_US
dc.identifier.isiWOS:000077780500031-
dc.publisher.placeUnited Kingdomen_US
dc.identifier.scopusauthoridSu, KYL=26326482200en_US
dc.identifier.scopusauthoridVolk, K=7006571965en_US
dc.identifier.scopusauthoridKwok, S=22980498300en_US
dc.identifier.scopusauthoridHrivnak, BJ=35613962100en_US

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