File Download
  Links for fulltext
     (May Require Subscription)
Supplementary

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
Su, KYLVolk, KKwok, SHrivnak, BJ
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?
DOI: http://dx.doi.org/10.1086/306449
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
0004-637X
2023 Impact Factor: 4.8
2023 SCImago Journal Rankings: 1.905
ISI Accession Number ID
WOS:000077780500031
References
References in Scopus

 

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.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
dc.identifier.issnl0004-637X-

Export via OAI-PMH Interface in XML Formats

OR

Export to Other Non-XML Formats