Resolving the electron temperature discrepancies in H II regions and planetary nebulae: κ-Distributed electrons

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dc.contributor.authorNicholls , David
dc.contributor.authorDopita, Michael
dc.contributor.authorSutherland, Ralph
dc.date.accessioned2015-12-10T23:06:30Z
dc.date.issued2012
dc.date.updated2016-02-24T09:33:46Z
dc.description.abstractThe measurement of electron temperatures and metallicities in H II regions and planetary nebulae (PNe) has - for several decades - presented a problem: results obtained using different techniques disagree. What is worse, they disagree consistently. There
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/62692
dc.publisherIOP Publishing
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: acceleration of particles; atomic data; atomic processes; H ii regions; ISM: abundances; planetary nebulae: general; plasmas
dc.titleResolving the electron temperature discrepancies in H II regions and planetary nebulae: κ-Distributed electrons
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2
local.contributor.affiliationNicholls , David, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationDopita, Michael, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationSutherland, Ralph, College of Physical and Mathematical Sciences, ANU
local.contributor.authoremailu4628677@anu.edu.au
local.contributor.authoruidNicholls , David, u4628677
local.contributor.authoruidDopita, Michael, u7501303
local.contributor.authoruidSutherland, Ralph, u8517070
local.description.notesImported from ARIES
local.identifier.absfor020100 - ASTRONOMICAL AND SPACE SCIENCES
local.identifier.ariespublicationf5625xPUB726
local.identifier.citationvolume752
local.identifier.doi10.1088/0004-637X/752/2/148
local.identifier.scopusID2-s2.0-84862208865
local.identifier.thomsonID000305738000071
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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