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Conference Paper: Circumstellar materials of SN 1987A

TitleCircumstellar materials of SN 1987A
Authors
Pun, CSJ
KeywordsCircumstellar materials
Supemovae
Supernova remnants
Issue Date2007
PublisherAmerican Institute of Physics.
Citation
Supernova 1987A: 20 Years After, Supernovae and Gamma-Ray Bursters. In AIP Conference Proceedings, 2007, v. 937 n. 1, p. 171-175 How to Cite?
DOI: http://dx.doi.org/10.1063/1.3682898
AbstractThe geometric and physical properties of the circumstellar materials of SN 1987A were studied. The detailed structure of the SN 1987A equatorial inner ring (EIR) was investigated using two dimensional spectral images of the ring obtained on 1997 December 9 (day 3942) with the Space Telescope Imaging Spectrograph (STIS) of the Hubble Space Telescope (HST). The data provided a valuable snapshot of the ring before foil fledge interaction with the supernova debris started. Geometric parameters of the EIR were determined for neutral and low-ionization emission line species of H, He, O, N, S, and Ne. We also investigated the electron temperature, density, and elemental abundances around the EIR and we found no azimuthal variation around the ring. © 2007 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/109736
ISSN
0094-243X
2023 SCImago Journal Rankings: 0.152
References
References in Scopus

 

DC FieldValueLanguage
dc.contributor.authorPun, CSJen_HK
dc.date.accessioned2010-09-26T01:35:02Z-
dc.date.available2010-09-26T01:35:02Z-
dc.date.issued2007en_HK
dc.identifier.citationSupernova 1987A: 20 Years After, Supernovae and Gamma-Ray Bursters. In AIP Conference Proceedings, 2007, v. 937 n. 1, p. 171-175en_HK
dc.identifier.issn0094-243Xen_HK
dc.identifier.urihttp://hdl.handle.net/10722/109736-
dc.description.abstractThe geometric and physical properties of the circumstellar materials of SN 1987A were studied. The detailed structure of the SN 1987A equatorial inner ring (EIR) was investigated using two dimensional spectral images of the ring obtained on 1997 December 9 (day 3942) with the Space Telescope Imaging Spectrograph (STIS) of the Hubble Space Telescope (HST). The data provided a valuable snapshot of the ring before foil fledge interaction with the supernova debris started. Geometric parameters of the EIR were determined for neutral and low-ionization emission line species of H, He, O, N, S, and Ne. We also investigated the electron temperature, density, and elemental abundances around the EIR and we found no azimuthal variation around the ring. © 2007 American Institute of Physics.en_HK
dc.languageengen_HK
dc.publisherAmerican Institute of Physics.en_HK
dc.relation.ispartofAIP Conference Proceedingsen_HK
dc.subjectCircumstellar materialsen_HK
dc.subjectSupemovaeen_HK
dc.subjectSupernova remnantsen_HK
dc.titleCircumstellar materials of SN 1987Aen_HK
dc.typeConference_Paperen_HK
dc.identifier.emailPun, CSJ: jcspun@hkucc.hku.hken_HK
dc.identifier.authorityPun, CSJ=rp00772en_HK
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.3682898en_HK
dc.identifier.scopuseid_2-s2.0-36849057517en_HK
dc.identifier.hkuros141917en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-36849057517&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume937en_HK
dc.identifier.issue1-
dc.identifier.spage171en_HK
dc.identifier.epage175en_HK
dc.publisher.placeUnited Statesen_HK
dc.identifier.scopusauthoridPun, CSJ=7003931846en_HK
dc.identifier.issnl0094-243X-

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