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Conference Paper: [Fe iii] lines in the planetary nebula NGC 2392

Title[Fe iii] lines in the planetary nebula NGC 2392
Authors
Zhang, YFang, XChau, WCHsia, CHLiu, XWKwok, S
Keywordsplanetary nebulae: individual (NGC 2392, Mz 3)
line: identification
Issue Date2011
PublisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAU
Citation
IAU Symposium No. 283: Planetary Nebulae: An Eye to the Future, Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 532-533 How to Cite?
DOI: http://dx.doi.org/10.1017/S1743921312012288
AbstractThe Eskimo Nebula (NGC 2392) is a young double-shell planetary nebula (PN). Its intrinsic structure and the responsible shaping mechanism are still not fully understood. We present new optical spectroscopy of NGC 2392 at two different locations to obtain the spectra of the inner and outer shells. Several [Fe iii] lines are clearly detected. We find that these [Fe iii] lines mostly originate from the inner shell. Therefore, we suggest that NGC 2392 might have an intrinsic structure similar to the Ant Nebula Mz 3, which exhibits a number of [Fe iii] lines from the central dense regions. In this scenario, the inner and outer shells correspond to the central emission core and the outer lobes of Mz 3, respectively. © 2012 International Astronomical Union.
Persistent Identifierhttp://hdl.handle.net/10722/165696
ISSN
1743-9213
2020 SCImago Journal Rankings: 0.124
ISI Accession Number ID
WOS:000309944800169

 

DC FieldValueLanguage
dc.contributor.authorZhang, Yen_HK
dc.contributor.authorFang, Xen_HK
dc.contributor.authorChau, WCen_HK
dc.contributor.authorHsia, CHen_HK
dc.contributor.authorLiu, XWen_HK
dc.contributor.authorKwok, Sen_HK
dc.date.accessioned2012-09-20T08:22:14Z-
dc.date.available2012-09-20T08:22:14Z-
dc.date.issued2011en_HK
dc.identifier.citationIAU Symposium No. 283: Planetary Nebulae: An Eye to the Future, Puerto de la Cruz, Tenerife, Spain, 25-29 July 2011. In International Astronomical Union Proceedings, 2011, v. 7 n. S283, p. 532-533en_US
dc.identifier.issn1743-9213en_HK
dc.identifier.urihttp://hdl.handle.net/10722/165696-
dc.description.abstractThe Eskimo Nebula (NGC 2392) is a young double-shell planetary nebula (PN). Its intrinsic structure and the responsible shaping mechanism are still not fully understood. We present new optical spectroscopy of NGC 2392 at two different locations to obtain the spectra of the inner and outer shells. Several [Fe iii] lines are clearly detected. We find that these [Fe iii] lines mostly originate from the inner shell. Therefore, we suggest that NGC 2392 might have an intrinsic structure similar to the Ant Nebula Mz 3, which exhibits a number of [Fe iii] lines from the central dense regions. In this scenario, the inner and outer shells correspond to the central emission core and the outer lobes of Mz 3, respectively. © 2012 International Astronomical Union.en_HK
dc.languageengen_US
dc.publisherCambridge University Press. The Journal's web site is located at http://journals.cambridge.org/action/displayJournal?jid=IAUen_HK
dc.relation.ispartofInternational Astronomical Union Proceedingsen_HK
dc.rightsInternational Astronomical Union Proceedings. Copyright © Cambridge University Press.-
dc.subjectplanetary nebulae: individual (NGC 2392, Mz 3)en_HK
dc.subjectline: identificationen_HK
dc.title[Fe iii] lines in the planetary nebula NGC 2392en_HK
dc.typeConference_Paperen_HK
dc.identifier.emailZhang, Y: zhangy96@hku.hken_HK
dc.identifier.emailChau, WC: e92m3@hku.hken_HK
dc.identifier.emailKwok, S: deannote@hku.hk-
dc.identifier.authorityZhang, Y=rp00841en_HK
dc.identifier.authorityKwok, S=rp00716en_HK
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1017/S1743921312012288en_HK
dc.identifier.scopuseid_2-s2.0-84865705257en_HK
dc.identifier.hkuros209392en_US
dc.identifier.volume7en_HK
dc.identifier.issueS283en_HK
dc.identifier.spage532en_HK
dc.identifier.epage533en_HK
dc.identifier.isiWOS:000309944800169-
dc.publisher.placeUnited Kingdomen_HK
dc.identifier.scopusauthoridKwok, S=22980498300en_HK
dc.identifier.scopusauthoridLiu, XW=51564252300en_HK
dc.identifier.scopusauthoridHsia, CH=55351470000en_HK
dc.identifier.scopusauthoridChau, W=55295678300en_HK
dc.identifier.scopusauthoridFang, X=55351718000en_HK
dc.identifier.scopusauthoridZhang, Y=23768446500en_HK
dc.customcontrol.immutablesml 130515-
dc.identifier.issnl1743-9213-

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