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Article: Spectroscopic and photometric observations of SN1987A. V - Days 386-616

TitleSpectroscopic and photometric observations of SN1987A. V - Days 386-616
Authors
KeywordsAstronomical Photometry
Magellanic Clouds
Spectroscopic Analysis
Supernova 1987a
Ubv Spectra
Bolometers
Cassegrain Optics
Energy Sources
X Ray Sources
Issue Date1989
PublisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 1989, v. 237, p. 55P-68P How to Cite?
AbstractSpectroscopic and photometric observations are presented of SN1987A in the Large Magellanic Cloud made between days 386 and 616 after the Kamiokande-II neutrino event. During this period the bolometric flux from the supernova measured over the U to M wavelength range has continued to decline faster than the Co-56 decay rate. By day 560 the flux in this wavelength range accounts for only half of that expected from Co-56 decay. The estimated total flux is consistent with Co-56 remaining the sole energy source of the supernova over the period considered.
Persistent Identifierhttp://hdl.handle.net/10722/211174
ISSN
2015 Impact Factor: 4.952
2015 SCImago Journal Rankings: 2.806

 

DC FieldValueLanguage
dc.contributor.authorCatchpole, RM-
dc.contributor.authorWhitelock, PA-
dc.contributor.authorMenzies, JW-
dc.contributor.authorFeast, MW-
dc.contributor.authorMarang, F-
dc.contributor.authorSekiguchi, K-
dc.contributor.authorvan Wyk, F-
dc.contributor.authorRoberts, G-
dc.contributor.authorBalona, LA-
dc.contributor.authorEgan, JM-
dc.contributor.authorCarter, BS-
dc.contributor.authorLaney, CD-
dc.contributor.authorLaing, JD-
dc.contributor.authorSpencer Jones, JH-
dc.contributor.authorGlass, IS-
dc.contributor.authorWinkler, H-
dc.contributor.authorFairall, AP-
dc.contributor.authorLloyd Evans, THH-
dc.contributor.authorCropper, MS-
dc.contributor.authorShenton, M-
dc.contributor.authorHill, PW-
dc.contributor.authorPayne, P-
dc.contributor.authorJones, KN-
dc.contributor.authorWargau, W-
dc.contributor.authorMason, KO-
dc.contributor.authorJeffery, CS-
dc.contributor.authorHellier, C-
dc.contributor.authorParker, QA-
dc.contributor.authorChini, R-
dc.contributor.authorJames, PA-
dc.contributor.authorDoyle, JG-
dc.contributor.authorButler, CJ-
dc.contributor.authorBromage, G-
dc.date.accessioned2015-07-08T03:22:35Z-
dc.date.available2015-07-08T03:22:35Z-
dc.date.issued1989-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1989, v. 237, p. 55P-68P-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/211174-
dc.description.abstractSpectroscopic and photometric observations are presented of SN1987A in the Large Magellanic Cloud made between days 386 and 616 after the Kamiokande-II neutrino event. During this period the bolometric flux from the supernova measured over the U to M wavelength range has continued to decline faster than the Co-56 decay rate. By day 560 the flux in this wavelength range accounts for only half of that expected from Co-56 decay. The estimated total flux is consistent with Co-56 remaining the sole energy source of the supernova over the period considered.-
dc.languageeng-
dc.publisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectAstronomical Photometry-
dc.subjectMagellanic Clouds-
dc.subjectSpectroscopic Analysis-
dc.subjectSupernova 1987a-
dc.subjectUbv Spectra-
dc.subjectBolometers-
dc.subjectCassegrain Optics-
dc.subjectEnergy Sources-
dc.subjectX Ray Sources-
dc.titleSpectroscopic and photometric observations of SN1987A. V - Days 386-616-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume237-
dc.identifier.spage55P-
dc.identifier.epage68P-

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