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Conference Paper: The 3D structure of the Ring nebula

TitleThe 3D structure of the Ring nebula
Authors
Steffen, WLópez, JAKoning, NKwok, SRiesgo, HRicher, MGMorisset, C
KeywordsM57
Ring nebula
Kinematics
3D modeling
Software
Issue Date2009
PublisherI.A.C. electronic publication.
Citation
The Asymmetric Planetary Nebulae 4 (APN4) Conference, La Palma, Spain, 18-22 June 2007. In Proceedings of Asymmetric Planetary Nebulae 4, 2009, p. 265-269 How to Cite?
AbstractThe Ring nebula (M57) is one of the closest and best observed planetary nebulae. Still, its structure remains controversial. Based on detailed spectroscopic observations of the kinematics we present a solution generated with SHAPE to the 3D structure of the [NII] emission. Assuming that the inner halo is the result from enhanced illumination from the central star through the holes of the inner nebula, we solve the geometry of the nebula.
DescriptionPart I: Asymmetry in the Planetary Nebula phase
Persistent Identifierhttp://hdl.handle.net/10722/128484

 

DC FieldValueLanguage
dc.contributor.authorSteffen, Wen_HK
dc.contributor.authorLópez, JAen_HK
dc.contributor.authorKoning, Nen_HK
dc.contributor.authorKwok, Sen_HK
dc.contributor.authorRiesgo, Hen_HK
dc.contributor.authorRicher, MGen_HK
dc.contributor.authorMorisset, Cen_HK
dc.date.accessioned2010-10-31T14:30:45Z-
dc.date.available2010-10-31T14:30:45Z-
dc.date.issued2009en_HK
dc.identifier.citationThe Asymmetric Planetary Nebulae 4 (APN4) Conference, La Palma, Spain, 18-22 June 2007. In Proceedings of Asymmetric Planetary Nebulae 4, 2009, p. 265-269en_HK
dc.identifier.urihttp://hdl.handle.net/10722/128484-
dc.descriptionPart I: Asymmetry in the Planetary Nebula phase-
dc.description.abstractThe Ring nebula (M57) is one of the closest and best observed planetary nebulae. Still, its structure remains controversial. Based on detailed spectroscopic observations of the kinematics we present a solution generated with SHAPE to the 3D structure of the [NII] emission. Assuming that the inner halo is the result from enhanced illumination from the central star through the holes of the inner nebula, we solve the geometry of the nebula.-
dc.languageengen_HK
dc.publisherI.A.C. electronic publication.en_HK
dc.relation.ispartofProceedings of Asymmetric Planetary Nebulae 4en_HK
dc.subjectM57-
dc.subjectRing nebula-
dc.subjectKinematics-
dc.subject3D modeling-
dc.subjectSoftware-
dc.titleThe 3D structure of the Ring nebulaen_HK
dc.typeConference_Paperen_HK
dc.identifier.emailSteffen, W: wsteffen@astrosen.unam.mxen_HK
dc.identifier.emailKwok, S: sunkwok@hku.hk-
dc.identifier.authorityKwok, S=rp00716en_HK
dc.description.naturelink_to_OA_fulltext-
dc.identifier.hkuros181554en_HK
dc.identifier.spage265en_HK
dc.identifier.epage269en_HK
dc.description.otherThe Asymmetric Planetary Nebulae 4 (APN4) Conference, La Palma, Spain, 18-22 June 2007. In Proceedings of Asymmetric Planetary Nebulae 4, 2009, p. 265-269-

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